diff --git a/paper/JOSS/paper.bib b/paper/JOSS/paper.bib index e4012a4..ae5d7db 100644 --- a/paper/JOSS/paper.bib +++ b/paper/JOSS/paper.bib @@ -1,7 +1,7 @@ @ARTICLE{Duchene+2013, author = {{Duch{\^e}ne}, Gaspard and {Kraus}, Adam}, - title = "{Stellar Multiplicity}", - journal = {\araa}, + title = {Stellar Multiplicity}, + journal = {Annual Reviews in Astronomy & Astrophysics}, keywords = {Astrophysics - Solar and Stellar Astrophysics}, year = 2013, month = aug, @@ -18,8 +18,8 @@ @ARTICLE{Duchene+2013 @ARTICLE{Moe+2017, author = {{Moe}, Maxwell and {Di Stefano}, Rosanne}, - title = "{Mind Your Ps and Qs: The Interrelation between Period (P) and Mass-ratio (Q) Distributions of Binary Stars}", - journal = {\apjs}, + title = {Mind Your {P}s and {Q}s: The Interrelation between Period ({P}) and Mass-ratio ({Q}) Distributions of Binary Stars}, + journal = {The Astrophysical Journal Supplement Series}, keywords = {binaries: close, binaries: general, stars: evolution, stars: formation, stars: massive, stars: statistics, Astrophysics - Solar and Stellar Astrophysics}, year = 2017, month = jun, @@ -37,7 +37,7 @@ @ARTICLE{Moe+2017 @INPROCEEDINGS{Offner+2023, author = {{Offner}, S.~S.~R. and {Moe}, M. and {Kratter}, K.~M. and {Sadavoy}, S.~I. and {Jensen}, E.~L.~N. and {Tobin}, J.~J.}, - title = "{The Origin and Evolution of Multiple Star Systems}", + title = {The Origin and Evolution of Multiple Star Systems}, keywords = {Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Astrophysics of Galaxies}, booktitle = {Protostars and Planets VII}, year = 2023, @@ -57,8 +57,8 @@ @INPROCEEDINGS{Offner+2023 @ARTICLE{Podsiadlowski+1992, author = {{Podsiadlowski}, Ph. and {Joss}, P.~C. and {Hsu}, J.~J.~L.}, - title = "{Presupernova Evolution in Massive Interacting Binaries}", - journal = {\apj}, + title = {Presupernova Evolution in Massive Interacting Binaries}, + journal = {The Astrophysical Journal}, keywords = {Binary Stars, Massive Stars, Stellar Evolution, Supernovae, Computational Astrophysics, Monte Carlo Method, Stellar Envelopes, Stellar Mass Accretion, Stellar Models, Supernova 1987a, Astrophysics}, year = 1992, month = may, @@ -71,7 +71,7 @@ @ARTICLE{Podsiadlowski+1992 @ARTICLE{Sana+2012, author = {{Sana}, H. and {de Mink}, S.~E. and {de Koter}, A. and {Langer}, N. and {Evans}, C.~J. and et al.}, - title = "{Binary Interaction Dominates the Evolution of Massive Stars}", + title = {Binary Interaction Dominates the Evolution of Massive Stars}, journal = {Science}, keywords = {ASTRONOMY, Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Cosmology and Extragalactic Astrophysics}, year = 2012, @@ -90,8 +90,8 @@ @ARTICLE{Sana+2012 @ARTICLE{deMink+2014, author = {{de Mink}, S.~E. and {Sana}, H. and {Langer}, N. and {Izzard}, R.~G. and {Schneider}, F.~R.~N.}, - title = "{The Incidence of Stellar Mergers and Mass Gainers among Massive Stars}", - journal = {\apj}, + title = {The Incidence of Stellar Mergers and Mass Gainers among Massive Stars}, + journal = {The Astrophysical Journal}, keywords = {binaries: close, Galaxy: stellar content, stars: early-type, stars: massive, Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Cosmology and Nongalactic Astrophysics}, year = 2014, month = feb, @@ -109,8 +109,8 @@ @ARTICLE{deMink+2014 @ARTICLE{Dekel+1986, author = {{Dekel}, A. and {Silk}, J.}, - title = "{The Origin of Dwarf Galaxies, Cold Dark Matter, and Biased Galaxy Formation}", - journal = {\apj}, + title = {The Origin of Dwarf Galaxies, Cold Dark Matter, and Biased Galaxy Formation}, + journal = {The Astrophysical Journal}, keywords = {Abundance, Cold Plasmas, Dark Matter, Dwarf Galaxies, Galactic Evolution, Stellar Winds, Virgo Galactic Cluster, Big Bang Cosmology, Galactic Structure, Local Group (Astronomy), Mass To Light Ratios, Stellar Evolution, Supernovae, Astrophysics, COSMOLOGY, GALAXIES: CLUSTERING, GALAXIES: FORMATION, GALAXIES: INTERNAL MOTIONS, GALAXIES: STRUCTURE}, year = 1986, month = apr, @@ -124,7 +124,7 @@ @ARTICLE{Dekel+1986 @ARTICLE{Hopkins+2012, author = {{Hopkins}, Philip F. and {Quataert}, Eliot and {Murray}, Norman}, title = "{Stellar feedback in galaxies and the origin of galaxy-scale winds}", - journal = {\mnras}, + journal = {Monthly Notices of the Royal Astronomical Society}, keywords = {stars: formation, galaxies: active, galaxies: evolution, galaxies: formation, cosmology: theory, Astrophysics - Cosmology and Extragalactic Astrophysics, Astrophysics - Galaxy Astrophysics, Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Solar and Stellar Astrophysics}, year = 2012, month = apr, @@ -141,8 +141,8 @@ @ARTICLE{Hopkins+2012 @ARTICLE{Naab+2017, author = {{Naab}, Thorsten and {Ostriker}, Jeremiah P.}, - title = "{Theoretical Challenges in Galaxy Formation}", - journal = {\araa}, + title = {Theoretical Challenges in Galaxy Formation}, + journal = {Annual Reviews in Astronomy & Astrophysics}, keywords = {Astrophysics - Astrophysics of Galaxies}, year = 2017, month = aug, @@ -159,8 +159,8 @@ @ARTICLE{Naab+2017 @ARTICLE{Nomoto+2013, author = {{Nomoto}, Ken'ichi and {Kobayashi}, Chiaki and {Tominaga}, Nozomu}, - title = "{Nucleosynthesis in Stars and the Chemical Enrichment of Galaxies}", - journal = {\araa}, + title = {Nucleosynthesis in Stars and the Chemical Enrichment of Galaxies}, + journal = {Annual Reviews in Astronomy & Astrophysics}, year = 2013, month = aug, volume = {51}, @@ -173,7 +173,7 @@ @ARTICLE{Nomoto+2013 @BOOK{Ivanova+2020, author = {{Ivanova}, Natalia and {Justham}, Stephen and {Ricker}, Paul}, - title = "{Common Envelope Evolution}", + title = {Common Envelope Evolution}, year = 2020, doi = {10.1088/2514-3433/abb6f0}, adsurl = {https://ui.adsabs.harvard.edu/abs/2020cee..book.....I}, @@ -201,7 +201,7 @@ @ARTICLE{Ropke+2023 @ARTICLE{Janka+2012, author = {{Janka}, Hans-Thomas}, - title = "{Explosion Mechanisms of Core-Collapse Supernovae}", + title = {Explosion Mechanisms of Core-Collapse Supernovae}, journal = {Annual Review of Nuclear and Particle Science}, keywords = {Astrophysics - Solar and Stellar Astrophysics, General Relativity and Quantum Cosmology, High Energy Physics - Phenomenology, Nuclear Theory}, year = 2012, @@ -219,8 +219,8 @@ @ARTICLE{Janka+2012 @ARTICLE{Somerville+2015, author = {{Somerville}, Rachel S. and {Dav{\'e}}, Romeel}, - title = "{Physical Models of Galaxy Formation in a Cosmological Framework}", - journal = {\araa}, + title = {Physical Models of Galaxy Formation in a Cosmological Framework}, + journal = {Annual Reviews in Astronomy & Astrophysics}, keywords = {Astrophysics - Astrophysics of Galaxies}, year = 2015, month = aug, @@ -237,7 +237,7 @@ @ARTICLE{Somerville+2015 @ARTICLE{Eldridge+2011, author = {{Eldridge}, John J. and {Langer}, Norbert and {Tout}, Christopher A.}, title = "{Runaway stars as progenitors of supernovae and gamma-ray bursts}", - journal = {\mnras}, + journal = {Monthly Notices of the Royal Astronomical Society}, keywords = {binaries: general, stars: evolution, gamma-ray burst: general, stars: massive, supernovae: general, stars: Wolf-Rayet, Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Cosmology and Nongalactic Astrophysics, Astrophysics - Astrophysics of Galaxies}, year = 2011, month = jul, @@ -255,7 +255,7 @@ @ARTICLE{Eldridge+2011 @ARTICLE{Renzo+2019, author = {{Renzo}, M. and {Zapartas}, E. and {de Mink}, S.~E. and {G{\"o}tberg}, Y. and {Justham}, S. and {Farmer}, R.~J. and {Izzard}, R.~G. and {Toonen}, S. and {Sana}, H.}, title = "{Massive runaway and walkaway stars. A study of the kinematical imprints of the physical processes governing the evolution and explosion of their binary progenitors}", - journal = {\aap}, + journal = {Astronomy & Astrophysics}, keywords = {astrometry, binaries: close, stars: evolution, stars: kinematics and dynamics, stars: massive, supernovae: general, Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Astrophysics of Galaxies}, year = 2019, month = apr, @@ -273,7 +273,7 @@ @ARTICLE{Renzo+2019 @ARTICLE{Disberg+2024, author = {{Disberg}, P. and {Gaspari}, N. and {Levan}, A.~J.}, title = "{Deceleration of kicked objects due to the Galactic potential}", - journal = {\aap}, + journal = {Astronomy & Astrophysics}, keywords = {stars: kinematics and dynamics, pulsars: general, Galaxy: stellar content, Astrophysics - Astrophysics of Galaxies, Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Solar and Stellar Astrophysics}, year = 2024, month = jul, @@ -291,7 +291,7 @@ @ARTICLE{Disberg+2024 @ARTICLE{Repetto+2017, author = {{Repetto}, Serena and {Igoshev}, Andrei P. and {Nelemans}, Gijs}, title = "{The Galactic distribution of X-ray binaries and its implications for compact object formation and natal kicks}", - journal = {\mnras}, + journal = {Monthly Notices of the Royal Astronomical Society}, keywords = {X-rays: binaries, supernovae: general, Galaxy: dynamics, binaries: general, black hole physics, stars: neutron, Astrophysics - High Energy Astrophysical Phenomena}, year = 2017, month = may, @@ -309,7 +309,7 @@ @ARTICLE{Repetto+2017 @ARTICLE{Mandel+2016, author = {{Mandel}, Ilya}, title = "{Estimates of black hole natal kick velocities from observations of low-mass X-ray binaries}", - journal = {\mnras}, + journal = {Monthly Notices of the Royal Astronomical Society}, keywords = {binaries: close, stars: black holes, Galaxy: kinematics and dynamics, X-rays: binaries, Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Astrophysics of Galaxies, Astrophysics - Solar and Stellar Astrophysics}, year = 2016, month = feb, @@ -327,7 +327,7 @@ @ARTICLE{Mandel+2016 @ARTICLE{Repetto+2012, author = {{Repetto}, Serena and {Davies}, Melvyn B. and {Sigurdsson}, Steinn}, title = "{Investigating stellar-mass black hole kicks}", - journal = {\mnras}, + journal = {Monthly Notices of the Royal Astronomical Society}, keywords = {black hole physics, binaries: general, stars: neutron, supernovae: general, Galaxy: kinematics and dynamics, X-rays: binaries, Astrophysics - Galaxy Astrophysics, Astrophysics - High Energy Astrophysical Phenomena}, year = 2012, month = oct, @@ -345,7 +345,7 @@ @ARTICLE{Repetto+2012 @ARTICLE{Repetto+2015, author = {{Repetto}, Serena and {Nelemans}, Gijs}, title = "{Constraining the formation of black holes in short-period black hole low-mass X-ray binaries}", - journal = {\mnras}, + journal = {Monthly Notices of the Royal Astronomical Society}, keywords = {black hole physics, binaries: general, stars: black holes, supernovae: general, X-rays: binaries, Astrophysics - High Energy Astrophysical Phenomena}, year = 2015, month = nov, @@ -363,7 +363,7 @@ @ARTICLE{Repetto+2015 @ARTICLE{Neuhauser+2020, author = {{Neuh{\"a}user}, R. and {Gie{\ss}ler}, F. and {Hambaryan}, V.~V.}, title = "{A nearby recent supernova that ejected the runaway star {\ensuremath{\zeta}} Oph, the pulsar PSR B1706-16, and $^{60}$Fe found on Earth}", - journal = {\mnras}, + journal = {Monthly Notices of the Royal Astronomical Society}, keywords = {astrometry, stars: individual: {\ensuremath{\zeta}} Oph, PSR B1706-16, PSR B1929+10, 1H11255-567, stars: neutron, supernovae: general, X-rays: binaries, Astrophysics - High Energy Astrophysical Phenomena}, year = 2020, month = oct, @@ -381,7 +381,7 @@ @ARTICLE{Neuhauser+2020 @ARTICLE{Evans+2020, author = {{Evans}, F.~A. and {Renzo}, M. and {Rossi}, E.~M.}, title = "{Core-collapse supernovae in binaries as the origin of galactic hyper-runaway stars}", - journal = {\mnras}, + journal = {Monthly Notices of the Royal Astronomical Society}, keywords = {binaries: general, supernovae: general, stars: kinematics and dynamics, massive, Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Astrophysics of Galaxies, Astrophysics - High Energy Astrophysical Phenomena}, year = 2020, month = oct, @@ -399,7 +399,7 @@ @ARTICLE{Evans+2020 @ARTICLE{Blaauw+1961, author = {{Blaauw}, A.}, title = "{On the origin of the O- and B-type stars with high velocities (the ``run-away'' stars), and some related problems}", - journal = {\bain}, + journal = {Bulletin of the Astronomical Institutes of the Netherlands}, year = 1961, month = may, volume = {15}, @@ -411,7 +411,7 @@ @ARTICLE{Blaauw+1961 @ARTICLE{Ivanova+2013, author = {{Ivanova}, Natalia and {Justham}, S. and {Chen}, X. and {De Marco}, O. and {Fryer}, C.~L. and {Gaburov}, E. and {Ge}, H. and {Glebbeek}, E. and {Han}, Z. and {Li}, X. -D. and {Lu}, G. and {Marsh}, T. and {Podsiadlowski}, P. and {Potter}, A. and {Soker}, N. and {Taam}, R. and {Tauris}, T.~M. and {van den Heuvel}, E.~P.~J. and {Webbink}, R.~F.}, title = "{Common envelope evolution: where we stand and how we can move forward}", - journal = {\aapr}, + journal = {The Astronomy and Astrophysics Review}, keywords = {Close binaries, Stellar structure, interiors, evolution, Hydrodynamics, Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Solar and Stellar Astrophysics}, year = 2013, month = feb, @@ -428,8 +428,8 @@ @ARTICLE{Ivanova+2013 @ARTICLE{Katsuda+2018, author = {{Katsuda}, Satoru and {Morii}, Mikio and {Janka}, Hans-Thomas and {Wongwathanarat}, Annop and {Nakamura}, Ko and {Kotake}, Kei and {Mori}, Koji and {M{\"u}ller}, Ewald and {Takiwaki}, Tomoya and {Tanaka}, Masaomi and {Tominaga}, Nozomu and {Tsunemi}, Hiroshi}, - title = "{Intermediate-mass Elements in Young Supernova Remnants Reveal Neutron Star Kicks by Asymmetric Explosions}", - journal = {\apj}, + title = {Intermediate-mass Elements in Young Supernova Remnants Reveal Neutron Star Kicks by Asymmetric Explosions}, + journal = {The Astrophysical Journal}, keywords = {ISM: supernova remnants, methods: data analysis, stars: neutron, techniques: imaging spectroscopy, X-rays: general, Astrophysics - High Energy Astrophysical Phenomena}, year = 2018, month = mar, @@ -447,22 +447,22 @@ @ARTICLE{Katsuda+2018 @ARTICLE{Marchant2023, author = {{Marchant}, Pablo and {Bodensteiner}, Julia}, - title = "{The Evolution of Massive Binary Stars}", - journal = {arXiv e-prints}, - keywords = {Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Astrophysics of Galaxies, Astrophysics - High Energy Astrophysical Phenomena}, - year = 2023, - month = nov, - eid = {arXiv:2311.01865}, - pages = {arXiv:2311.01865}, - doi = {10.48550/arXiv.2311.01865}, + title = {The Evolution of Massive Binary Stars}, + journal = {Annual Reviews in Astronomy & Astrophysics}, + keywords = {massive stars, stellar evolution, rotation, compact objects, gravitational waves, Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Astrophysics of Galaxies, Astrophysics - High Energy Astrophysical Phenomena}, + year = 2024, + month = sep, + volume = {62}, + number = {1}, + pages = {21-61}, + doi = {10.1146/annurev-astro-052722-105936}, archivePrefix = {arXiv}, eprint = {2311.01865}, primaryClass = {astro-ph.SR}, - adsurl = {https://ui.adsabs.harvard.edu/abs/2023arXiv231101865M}, + adsurl = {https://ui.adsabs.harvard.edu/abs/2024ARA&A..62...21M}, adsnote = {Provided by the SAO/NASA Astrophysics Data System} } - @Article{ zapartas:17, author = "E. {Zapartas} and S.~E. {de Mink} and R.~G. {Izzard} and S.-C. {Yoon} and C. {Badenes} and Y. {G{\"o}tberg} and A. @@ -470,7 +470,7 @@ @Article{ zapartas:17 {Schootemeijer} and T.~S. {Shrotriya}", title = "{Delay-time distribution of core-collapse supernovae with late events resulting from binary interaction}", - journal = "\aap", + journal = "Astronomy & Astrophysics", archiveprefix = "arXiv", eprint = "1701.07032", primaryclass = "astro-ph.HE", @@ -489,7 +489,7 @@ @Article{ zapartas:17 @ARTICLE{atri:19, author = {{Atri}, P. and {Miller-Jones}, J.~C.~A. and {Bahramian}, A. and {Plotkin}, R.~M. and {Jonker}, P.~G. and {Nelemans}, G. and {Maccarone}, T.~J. and {Sivakoff}, G.~R. and {Deller}, A.~T. and {Chaty}, S. and {Torres}, M.~A.~P. and {Horiuchi}, S. and {McCallum}, J. and {Natusch}, T. and {Phillips}, C.~J. and {Stevens}, J. and {Weston}, S.}, title = "{Potential kick velocity distribution of black hole X-ray binaries and implications for natal kicks}", - journal = {\mnras}, + journal = {Monthly Notices of the Royal Astronomical Society}, keywords = {astrometry, parallaxes, proper motions, stars: kinematics and dynamics, X-rays: binaries, Astrophysics - High Energy Astrophysical Phenomena}, year = 2019, month = nov, @@ -507,7 +507,7 @@ @ARTICLE{atri:19 @ARTICLE{underworld, author = {{Sweeney}, David and {Tuthill}, Peter and {Sharma}, Sanjib and {Hirai}, Ryosuke}, title = "{The Galactic underworld: the spatial distribution of compact remnants}", - journal = {\mnras}, + journal = {Monthly Notices of the Royal Astronomical Society}, keywords = {methods: numerical, astrometry, proper motions, stars: abundances, stars: black holes, stars: neutron, Astrophysics - Astrophysics of Galaxies, Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Instrumentation and Methods for Astrophysics}, year = 2022, month = nov, @@ -525,7 +525,7 @@ @ARTICLE{underworld @ARTICLE{Sweeney+2024, author = {{Sweeney}, David and {Tuthill}, Peter and {Krone-Martins}, Alberto and {M{\'e}rand}, Antoine and {Scalzo}, Richard and {Martinod}, Marc-Antoine}, title = "{Observing the galactic underworld: predicting photometry and astrometry from compact remnant microlensing events}", - journal = {\mnras}, + journal = {Monthly Notices of the Royal Astronomical Society}, keywords = {Astrophysics - Astrophysics of Galaxies, Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Solar and Stellar Astrophysics}, year = 2024, month = jun, @@ -541,9 +541,9 @@ @ARTICLE{Sweeney+2024 } @ARTICLE{COMPAS, - author = {{Riley}, Jeff and {Agrawal}, Poojan and {Barrett}, Jim W. and {Boyett}, Kristan N.~K. and {Broekgaarden}, Floor S. and {Chattopadhyay}, Debatri and {Gaebel}, Sebastian M. and {Gittins}, Fabian and {Hirai}, Ryosuke and {Howitt}, George and {Justham}, Stephen and {Khandelwal}, Lokesh and {Kummer}, Floris and {Lau}, Mike Y.~M. and {Mandel}, Ilya and {de Mink}, Selma E. and {Neijssel}, Coenraad and {Riley}, Tim and {van Son}, Lieke and {Stevenson}, Simon and {Vigna-G{\'o}mez}, Alejandro and {Vinciguerra}, Serena and {Wagg}, Tom and {Willcox}, Reinhold and {Team Compas}}, - title = "{Rapid Stellar and Binary Population Synthesis with COMPAS}", - journal = {\apjs}, + author = {{Riley}, Jeff and {Agrawal}, Poojan and {Barrett}, Jim W. and {Boyett}, Kristan N.~K. and {Broekgaarden}, Floor S. and {Chattopadhyay}, Debatri and {Gaebel}, Sebastian M. and {Gittins}, Fabian and {Hirai}, Ryosuke and {Howitt}, George and {Justham}, Stephen and {Khandelwal}, Lokesh and {Kummer}, Floris and {Lau}, Mike Y.~M. and {Mandel}, Ilya and {de Mink}, Selma E. and {Neijssel}, Coenraad and {Riley}, Tim and {van Son}, Lieke and {Stevenson}, Simon and {Vigna-G{\'o}mez}, Alejandro and {Vinciguerra}, Serena and {Wagg}, Tom and {Willcox}, Reinhold and {Team COMPAS}}, + title = {Rapid Stellar and Binary Population Synthesis with {COMPAS}}, + journal = {The Astrophysical Journal Supplement Series}, keywords = {1622, 154, 1108, 162, Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Solar and Stellar Astrophysics}, year = 2022, month = feb, @@ -576,7 +576,7 @@ @ARTICLE{NIGO @ARTICLE{Chattopadhyay+2020, author = {{Chattopadhyay}, Debatri and {Stevenson}, Simon and {Hurley}, Jarrod R. and {Rossi}, Luca J. and {Flynn}, Chris}, title = "{Modelling double neutron stars: radio and gravitational waves}", - journal = {\mnras}, + journal = {Monthly Notices of the Royal Astronomical Society}, keywords = {gravitational waves, stars: neutron, pulsars: general, Astrophysics - High Energy Astrophysical Phenomena, General Relativity and Quantum Cosmology}, year = 2020, month = may, @@ -594,7 +594,7 @@ @ARTICLE{Chattopadhyay+2020 @ARTICLE{Chattopadhyay+2021, author = {{Chattopadhyay}, Debatri and {Stevenson}, Simon and {Hurley}, Jarrod R. and {Bailes}, Matthew and {Broekgaarden}, Floor}, title = "{Modelling neutron star-black hole binaries: future pulsar surveys and gravitational wave detectors}", - journal = {\mnras}, + journal = {Monthly Notices of the Royal Astronomical Society}, keywords = {gravitational waves, pulsars: general, black hole - neutron star mergers, Astrophysics - High Energy Astrophysical Phenomena, General Relativity and Quantum Cosmology}, year = 2021, month = jul, @@ -628,8 +628,8 @@ @ARTICLE{Song+2024 @ARTICLE{Andrews+2022, author = {{Andrews}, Jeff J. and {Kalogera}, Vicky}, - title = "{Constraining Black Hole Natal Kicks with Astrometric Microlensing}", - journal = {\apj}, + title = "{Constraining black hole natal kicks with astrometric microlensing}", + journal = {The Astrophysical Journal}, keywords = {Black hole physics, Binary stars, 159, 154, Astrophysics - High Energy Astrophysical Phenomena}, year = 2022, month = may, @@ -665,7 +665,7 @@ @ARTICLE{cogsworth_full @ARTICLE{Gaspari+2024a, author = {{Gaspari}, N. and {Levan}, Andrew J. and {Chrimes}, Ashley A. and {Nelemans}, Gijs}, title = "{The Galactic neutron star population - II. Systemic velocities and merger locations of binary neutron stars}", - journal = {\mnras}, + journal = {Monthly Notices of the Royal Astronomical Society}, keywords = {binaries: general, gamma-ray burst: general, stars: neutron, Galaxy: stellar content, Galaxy: structure, Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Solar and Stellar Astrophysics, General Relativity and Quantum Cosmology}, year = 2024, month = jan, @@ -683,7 +683,7 @@ @ARTICLE{Gaspari+2024a @ARTICLE{Disberg+2024b, author = {{Disberg}, P. and {Gaspari}, N. and {Levan}, A.~J.}, title = "{Kinematic constraints on the ages and kick velocities of Galactic neutron star binaries}", - journal = {\aap}, + journal = {Astronomy & Astrophysics}, keywords = {binaries: general, stars: kinematics and dynamics, Galaxy: stellar content, Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Astrophysics of Galaxies, Astrophysics - Solar and Stellar Astrophysics}, year = 2024, month = sep, @@ -703,7 +703,7 @@ @ARTICLE{Disberg+2024b @ARTICLE{Mandhai+2022, author = {{Mandhai}, S. and {Lamb}, G.~P. and {Tanvir}, N.~R. and {Bray}, J. and {Nixon}, C.~J. and {Eyles-Ferris}, R.~A.~J. and {Levan}, A.~J. and {Gompertz}, B.~P.}, title = "{Exploring compact binary merger host galaxies and environments with zELDA}", - journal = {\mnras}, + journal = {Monthly Notices of the Royal Astronomical Society}, keywords = {transients: gamma-ray bursts, transients: neutron star mergers, transient: black hole - neutron star mergers, galaxies: general, stars: kinematics and dynamics, binaries: close, Astrophysics - High Energy Astrophysical Phenomena}, year = 2022, month = aug, @@ -720,8 +720,8 @@ @ARTICLE{Mandhai+2022 @ARTICLE{Zevin+2020, author = {{Zevin}, Michael and {Kelley}, Luke Zoltan and {Nugent}, Anya and {Fong}, Wen-fai and {Berry}, Christopher P.~L. and {Kalogera}, Vicky}, - title = "{Forward Modeling of Double Neutron Stars: Insights from Highly Offset Short Gamma-Ray Bursts}", - journal = {\apj}, + title = {Forward Modeling of Double Neutron Stars: Insights from Highly Offset Short Gamma-Ray Bursts}, + journal = {The Astrophysical Journal}, keywords = {Gamma-ray bursts, Supernova dynamics, Neutron stars, Compact binary stars, Stellar evolution, Galaxy evolution, 629, 1664, 1108, 283, 1599, 594, Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Astrophysics of Galaxies}, year = 2020, month = dec, diff --git a/paper/JOSS/paper.md b/paper/JOSS/paper.md index 66d6fd7..0983fa6 100644 --- a/paper/JOSS/paper.md +++ b/paper/JOSS/paper.md @@ -1,5 +1,5 @@ --- -title: 'cogsworth: A Gala of COSMIC Proportions Combining Binary Stellar Evolution and Galactic Dynamics' +title: 'cogsworth: A gala of COSMIC proportions combining binary stellar evolution and galactic dynamics' tags: - Python - astronomy @@ -19,7 +19,7 @@ authors: orcid: 0000-0003-0872-7098 affiliation: "2" affiliations: - - name: Department of Astronomy, University of Washington, Seattle, WA, 98195 + - name: Department of Astronomy, University of Washington, Seattle, WA, 98195, USA index: 1 - name: Center for Computational Astrophysics, Flatiron Institute, 162 Fifth Ave, New York, NY, 10010, USA index: 2 @@ -27,7 +27,7 @@ affiliations: index: 3 - name: University of Arizona, Department of Astronomy \& Steward Observatory, 933 N. Cherry Ave., Tucson, AZ 85721, USA index: 4 -date: 06 Septemeber 2024 +date: 06 September 2024 bibliography: paper.bib # Optional fields if submitting to a AAS journal too, see this blog post: @@ -38,22 +38,22 @@ aas-journal: Astrophysical Journal Supplement Series # Summary -We present `cogsworth`, an open-source Python tool for producing self-consistent population synthesis and galactic dynamics simulations. With `cogsworth` one can (1) sample a population of binaries and star formation history, (2) perform rapid (binary) stellar evolution, (3) integrate orbits through the galaxy and (4) inspect the full evolutionary history of each star or compact object, as well as its positions and kinematics. We include the functionality for post-processing hydrodynamical zoom-in simulations as a basis for galactic potentials and star formation histories to better account for initial spatial stellar clustering and more complex potentials. Alternatively, several analytical models are available for both the potential and star formation history. `cogsworth` can transform the intrinsic simulated population into an observed population through the joint application of dust maps, bolometric correction functions, and survey selection functions. This paper is jointly published in ApJS [@cogsworth_full]. +We present `cogsworth`, an open-source Python tool for producing self-consistent population synthesis and galactic dynamics simulations. With `cogsworth` one can (1) sample a population of binaries and star formation history, (2) perform rapid (binary) stellar evolution, (3) integrate orbits through the galaxy and (4) inspect the full evolutionary history of each star or compact object, as well as its position and kinematics. We include the functionality for post-processing hydrodynamical zoom-in simulations as a basis for galactic potentials and star formation histories to better account for initial spatial stellar clustering and more complex potentials. Alternatively, several analytical models are available for both the potential and star formation history. `cogsworth` can transform the intrinsic simulated population into an observed population through the joint application of dust maps, bolometric correction functions, and survey selection functions. # Statement of need -The majority of stars are born in binaries and multiple star systems (e.g., @Duchene+2013; @Moe+2017; @Offner+2023), a large subset of which will exchange mass at some point in their lives (e.g., @Podsiadlowski+1992; @Sana+2012; @deMink+2014). These massive stars play a critical role in the formation and evolution of galaxies as a result of their feedback (e.g., @Dekel+1986; @Hopkins+2012; @Nomoto+2013; @Somerville+2015; @Naab+2017). However, binary evolution remains uncertain, with many parameters such as common-envelope efficiency, mass transfer efficiency, angular momentum loss due to mass transfer and the mean magnitude of supernova natal kicks unconstrained over several orders of magnitude (e.g., @Janka+2012; @Ivanova+2013; @Katsuda+2018; @Ivanova+2020; @Ropke+2023; @Marchant2023). +The majority of stars are born in binaries and multiple star systems [e.g., @Duchene+2013; @Moe+2017; @Offner+2023], a large subset of which will exchange mass at some point in their lives [e.g., @deMink+2014; @Podsiadlowski+1992; @Sana+2012]. These massive stars play a critical role in the formation and evolution of galaxies as a result of their feedback [e.g., @Dekel+1986; @Hopkins+2012; @Nomoto+2013; @Somerville+2015; @Naab+2017]. However, binary evolution remains uncertain, with many parameters such as common-envelope efficiency, mass transfer efficiency, angular momentum loss due to mass transfer and the mean magnitude of supernova natal kicks unconstrained over several orders of magnitude [e.g., @Ivanova+2020; @Janka+2012; @Ivanova+2013; @Katsuda+2018; @Ropke+2023; @Marchant2023]. -Single massive stars are not expected to migrate far from their birth location before reaching core-collapse due to their short lifetimes ($\lesssim50$\,Myr, e.g., @zapartas:17). However, binary stars may disrupt after an initial supernova event, ejecting the secondary star from the system at its orbital velocity (e.g., @Blaauw+1961; @Eldridge+2011; @Renzo+2019). Thus, close massive binaries that disrupt can lead to the displacement of secondary stars significantly farther from star-forming regions. The present-day positions and kinematics of massive stars and binary products are therefore strongly impacted by changes in binary physics that alter the pre-supernova separation. This means that comparing simulations of positions and kinematics of stars and compact objects to observations will enable constraints on binary stellar evolution parameters. +Single massive stars are not expected to migrate far from their birth location before reaching core-collapse due to their short lifetimes [$\lesssim50$\,Myr, e.g., @zapartas:17]. However, binary stars may be disrupted after an initial supernova event, ejecting the secondary star from the system at its orbital velocity [e.g., @Blaauw+1961; @Eldridge+2011; @Renzo+2019]. Thus, close massive binaries that are disrupted can lead to the displacement of secondary stars significantly farther from star-forming regions. The present-day positions and kinematics of massive stars and binary products are therefore strongly impacted by changes in binary physics that alter the pre-supernova separation. This means that comparing simulations of positions and kinematics of stars and compact objects to observations will enable constraints on binary stellar evolution parameters. -The use of positions and kinematics as tracers of binary evolution has been considered in the past. Recent work has shown the importance of accounting for the galactic potential, which can change the velocity of kicked objects (e.g. @Disberg+2024). It is also important to consider the inclination or timing of a supernova kick relative to the galactic orbit, since, for example, a kick out of the galactic plane at an object's highest galactic vertical position will have a strong effect on its final position. Failing to consider impacts from both a galactic potential and kicks (i.e. velocity impulses) will lead to misleading conclusions regarding the final spatial distributions of the population. Some studies have considered using the Galactic potential at the present-day positions of objects to place a lower limit on the peculiar velocity at birth and constrain supernova kicks [@Repetto+2012; @Repetto+2015; @Repetto+2017; @atri:19], but the accuracy of this method is debated [@Mandel+2016]. Other works have considered the impact of the Galactic potential for individual special cases, rather than at a population level. For example, @Evans+2020 considered the orbits of hyper-runaway candidates evolving through the Milky Way potential, while @Neuhauser+2020 developed software for tracing the motion of stars to investigate the recent nearby supernovae that ejected $\zeta$ Ophiuchi. @Andrews+2022 considered galactic orbits of synthetic populations to place constraints on black hole natal kicks based on observations of a microlensed black hole. +The use of positions and kinematics as tracers of binary evolution has been considered in the past. Recent work has shown the importance of accounting for the galactic potential, which can change the velocity of kicked objects [e.g. @Disberg+2024]. It is also important to consider the inclination or timing of a supernova kick relative to the galactic orbit, since, for example, a kick out of the galactic plane at an object's highest galactic vertical position will have a strong effect on its final position. Failing to consider impacts from both a galactic potential and kicks (i.e. velocity impulses) will lead to misleading conclusions regarding the final spatial distributions of the population. Some studies have considered using the galactic potential at the present-day positions of objects to place a lower limit on the peculiar velocity at birth and constrain supernova kicks [@Repetto+2012; @Repetto+2015; @Repetto+2017; @atri:19], but the accuracy of this method is debated [@Mandel+2016]. Other works have considered the impact of the galactic potential for individual special cases, rather than at a population level. For example, @Evans+2020 considered the orbits of hyper-runaway candidates evolving through the Milky Way potential, while @Neuhauser+2020 developed software for tracing the motion of stars to investigate the recent nearby supernovae that ejected $\zeta$ Ophiuchi. @Andrews+2022 considered galactic orbits of synthetic populations to place constraints on black hole natal kicks based on observations of a microlensed black hole. -Additionally, there are several works that consider a full population of objects integrated through a galactic potential. @underworld and @Sweeney+2024 used a combination of `GALAXIA` and `galpy` to predict the spatial distribution of black holes and neutron stars in the Milky Way. Similarly, several works have combined population synthesis with galactic orbit integration (e.g. using `COMPAS` [@COMPAS] and `NIGO` [@NIGO]) to investigate binary neutron stars and pulsars [@Chattopadhyay+2020; @Chattopadhyay+2021; @Gaspari+2024a; @Disberg+2024b; @Song+2024], as well as binary neutron star mergers and short gamma-ray bursts [@Zevin+2020; @Mandhai+2022; @Gaspari+2024b]. +Additionally, there are several works that consider a full population of objects integrated through a galactic potential. @underworld and @Sweeney+2024 used a combination of `Galaxia` and `galpy` to predict the spatial distribution of black holes and neutron stars in the Milky Way. Similarly, several works have combined population synthesis with galactic orbit integration [e.g. using `COMPAS`, @COMPAS; and `NIGO`, @NIGO] to investigate binary neutron stars and pulsars [@Chattopadhyay+2020; @Chattopadhyay+2021; @Gaspari+2024a; @Disberg+2024b; @Song+2024], as well as binary neutron star mergers and short gamma-ray bursts [@Zevin+2020; @Mandhai+2022; @Gaspari+2024b]. -There is a clear need for a unified open-source tool that provides the theoretical infrastructure for making predictions for the positions and kinematics of massive stars and compact objects, placing these systems in the context of their host galaxy and its gravitational potential. `cogsworth` fulfills this need, providing a framework for self-consistent population synthesis and galactic dynamics simulations. The code is applicable to a wide range of binary products, both common and rare, from walkaway and runaway stars to X-ray binaries, as well as gravitational-wave and gamma-ray burst progenitors. +There is a clear need for a unified open-source tool that provides the theoretical infrastructure for making predictions for the positions and kinematics of massive stars and compact objects, placing these systems in the context of their host galaxy and its gravitational potential. `cogsworth` fulfils this need, providing a framework for self-consistent population synthesis and galactic dynamics simulations. The code is applicable to a wide range of binary products, both common and rare, from walkaway and runaway stars to X-ray binaries, as well as gravitational-wave and gamma-ray burst progenitors. # Acknowledgements We gratefully acknowledge many fruitful discussions with Julianne Dalcanton and Eric Bellm that resulted in several helpful suggestions. TW acknowledges valuable conversations with Matt Orr and Chris Hayward regarding the FIRE simulations, and with Alyson Brooks and Akaxia Cruz regarding the ChaNGa simulations. TW thanks the Simons Foundation, Flatiron Institute and Center for Computational Astrophysics for running the pre-doctoral program during which much of this work was completed. The Flatiron Institute is supported by the Simons Foundation. TW and KB acknowledge support from NASA ATP grant 80NSSC24K0768. -# References \ No newline at end of file +# References