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@ARTICLE{Paxton2011, | ||
author = {{Paxton}, B. and {Bildsten}, L. and {Dotter}, A. and {Herwig}, F. and {Lesaffre}, P. and {Timmes}, F.}, | ||
title = {{Modules for Experiments in Stellar Astrophysics (MESA)}}, | ||
journal = {\apjs}, | ||
archivePrefix = {arXiv}, | ||
eprint = {1009.1622}, | ||
primaryClass = {astro-ph.SR}, | ||
keywords = {methods: numerical, stars: evolution, stars: general}, | ||
year = {2011}, | ||
month = {jan}, | ||
volume = {192}, | ||
eid = {3}, | ||
pages = {3}, | ||
doi = {10.1088/0067-0049/192/1/3}, | ||
adsurl = {https://ui.adsabs.harvard.edu/abs/2011ApJS..192....3P}, | ||
adsnote = {Provided by the SAO/NASA Astrophysics Data System}, | ||
} | ||
|
||
@ARTICLE{Paxton2013, | ||
author = {{Paxton}, B. and {Cantiello}, M. and {Arras}, P. and {Bildsten}, L. and {Brown}, E.~F. and {Dotter}, A. and {Mankovich}, C. and {Montgomery}, M.~H. and {Stello}, D. and {Timmes}, F.~X. and {Townsend}, R.}, | ||
title = {{Modules for Experiments in Stellar Astrophysics (MESA): Planets, Oscillations, Rotation, and Massive Stars}}, | ||
journal = {\apjs}, | ||
archivePrefix = {arXiv}, | ||
eprint = {1301.0319}, | ||
primaryClass = {astro-ph.SR}, | ||
keywords = {asteroseismology, methods: numerical, planets and satellites: physical evolution, stars: evolution, stars: massive, stars: rotation}, | ||
year = {2013}, | ||
month = {sep}, | ||
volume = {208}, | ||
eid = {4}, | ||
pages = {4}, | ||
doi = {10.1088/0067-0049/208/1/4}, | ||
adsurl = {https://ui.adsabs.harvard.edu/abs/2013ApJS..208....4P}, | ||
adsnote = {Provided by the SAO/NASA Astrophysics Data System}, | ||
} | ||
|
||
@ARTICLE{Paxton2015, | ||
author = {{Paxton}, B. and {Marchant}, P. and {Schwab}, J. and {Bauer}, E.~B. and {Bildsten}, L. and {Cantiello}, M. and {Dessart}, L. and {Farmer}, R. and {Hu}, H. and {Langer}, N. and {Townsend}, R.~H.~D. and {Townsley}, D.~M. and {Timmes}, F.~X.}, | ||
title = {{Modules for Experiments in Stellar Astrophysics (MESA): Binaries, Pulsations, and Explosions}}, | ||
journal = {\apjs}, | ||
archivePrefix = {arXiv}, | ||
eprint = {1506.03146}, | ||
primaryClass = {astro-ph.SR}, | ||
keywords = {binaries: general, methods: numerical, nuclear reactions, nucleosynthesis, abundances, shock waves, stars: evolution, stars: oscillations}, | ||
year = {2015}, | ||
month = {sep}, | ||
volume = {220}, | ||
eid = {15}, | ||
pages = {15}, | ||
doi = {10.1088/0067-0049/220/1/15}, | ||
adsurl = {https://ui.adsabs.harvard.edu/abs/2015ApJS..220...15P}, | ||
adsnote = {Provided by the SAO/NASA Astrophysics Data System}, | ||
} | ||
|
||
@ARTICLE{Paxton2018, | ||
author = {{Paxton}, B. and {Schwab}, J. and {Bauer}, E.~B. and {Bildsten}, L. and {Blinnikov}, S. and {Duffell}, P. and {Farmer}, R. and {Goldberg}, J.~A. and {Marchant}, P. and {Sorokina}, E. and {Thoul}, A. and {Townsend}, R.~H.~D. and {Timmes}, F.~X.}, | ||
title = {{Modules for Experiments in Stellar Astrophysics (MESA): Convective Boundaries, Element Diffusion, and Massive Star Explosions}}, | ||
journal = {\apjs}, | ||
archivePrefix = {arXiv}, | ||
eprint = {1710.08424}, | ||
primaryClass = {astro-ph.SR}, | ||
keywords = {convection, diffusion, hydrodynamics, methods: numerical, stars: evolution, supernovae: general }, | ||
year = {2018}, | ||
month = {feb}, | ||
volume = {234}, | ||
eid = {34}, | ||
pages = {34}, | ||
doi = {10.3847/1538-4365/aaa5a8}, | ||
adsurl = {https://ui.adsabs.harvard.edu/abs/2018ApJS..234...34P}, | ||
adsnote = {Provided by the SAO/NASA Astrophysics Data System}, | ||
} | ||
|
||
@ARTICLE{Paxton2019, | ||
author = {{Paxton}, Bill and {Smolec}, R. and {Schwab}, Josiah and {Gautschy}, A. and | ||
{Bildsten}, Lars and {Cantiello}, Matteo and {Dotter}, Aaron and | ||
{Farmer}, R. and {Goldberg}, Jared A. and {Jermyn}, Adam S. and | ||
{Kanbur}, S.~M. and {Marchant}, Pablo and {Thoul}, Anne and | ||
{Townsend}, Richard H.~D. and {Wolf}, William M. and {Zhang}, Michael and | ||
{Timmes}, F.~X.}, | ||
title = "{Modules for Experiments in Stellar Astrophysics (MESA): Pulsating Variable Stars, Rotation, Convective Boundaries, and Energy Conservation}", | ||
journal = {\apjs}, | ||
keywords = {stars: evolution, stars: general, stars: interiors, stars: oscillations: including pulsations, stars: rotation, stars: variables: general, Astrophysics - Solar and Stellar Astrophysics}, | ||
year = "2019", | ||
month = "Jul", | ||
volume = {243}, | ||
number = {1}, | ||
eid = {10}, | ||
pages = {10}, | ||
doi = {10.3847/1538-4365/ab2241}, | ||
archivePrefix = {arXiv}, | ||
eprint = {1903.01426}, | ||
primaryClass = {astro-ph.SR}, | ||
adsurl = {https://ui.adsabs.harvard.edu/abs/2019ApJS..243...10P}, | ||
adsnote = {Provided by the SAO/NASA Astrophysics Data System} | ||
} | ||
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||
@ARTICLE{Jermyn2023, | ||
author = {{Jermyn}, Adam S. and {Bauer}, Evan B. and {Schwab}, Josiah and {Farmer}, R. and {Ball}, Warrick H. and {Bellinger}, Earl P. and {Dotter}, Aaron and {Joyce}, Meridith and {Marchant}, Pablo and {Mombarg}, Joey S.~G. and {Wolf}, William M. and {Sunny Wong}, Tin Long and {Cinquegrana}, Giulia C. and {Farrell}, Eoin and {Smolec}, R. and {Thoul}, Anne and {Cantiello}, Matteo and {Herwig}, Falk and {Toloza}, Odette and {Bildsten}, Lars and {Townsend}, Richard H.~D. and {Timmes}, F.~X.}, | ||
title = "{Modules for Experiments in Stellar Astrophysics (MESA): Time-dependent Convection, Energy Conservation, Automatic Differentiation, and Infrastructure}", | ||
journal = {\apjs}, | ||
keywords = {Stellar physics, Stellar evolution, Stellar evolutionary models, Computational methods, 1621, 1599, 2046, 1965, Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Instrumentation and Methods for Astrophysics}, | ||
year = 2023, | ||
month = mar, | ||
volume = {265}, | ||
number = {1}, | ||
eid = {15}, | ||
pages = {15}, | ||
doi = {10.3847/1538-4365/acae8d}, | ||
archivePrefix = {arXiv}, | ||
eprint = {2208.03651}, | ||
primaryClass = {astro-ph.SR}, | ||
adsurl = {https://ui.adsabs.harvard.edu/abs/2023ApJS..265...15J}, | ||
adsnote = {Provided by the SAO/NASA Astrophysics Data System} | ||
} |
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