Modelling the evolution of solar-mass stars with a range of metallicities using MESA
The nuclides 1,2H, 3,4He, 7Li, 7Be, 8B, 12,13C, 13-15N, 14-18O, 17-19F, 18-22Ne, 22Mg, and 24Mg were used in the code package MESA (Modules for Experiments in Stellar Astrophysics)[Paxton] to model a one-solar-mass star with a range of metallicities, z, from 0 to 0.1. On HR diagrams of each star mod...
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Online Access: | http://dx.doi.org/10.1051/epjconf/20159303011 |
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doaj-41bf6de705dc4b799b97135bd9610f362021-08-02T07:44:40ZengEDP SciencesEPJ Web of Conferences2100-014X2015-01-01930301110.1051/epjconf/20159303011epjconf_cgs2015_03011Modelling the evolution of solar-mass stars with a range of metallicities using MESAJones E.F.Gore P.M.The nuclides 1,2H, 3,4He, 7Li, 7Be, 8B, 12,13C, 13-15N, 14-18O, 17-19F, 18-22Ne, 22Mg, and 24Mg were used in the code package MESA (Modules for Experiments in Stellar Astrophysics)[Paxton] to model a one-solar-mass star with a range of metallicities, z, from 0 to 0.1. On HR diagrams of each star models luminosity and effective temperature from before zero-age main sequence (pre-ZAMS) to white dwarf, oscillations were noted in the horizontal branch at intervals from z = 0 to 0.0070. At z, = 0, the calculated stellar lifetime is 6.09x109 years. The calculated lifetime of the model stars increases to a maximum of 1.25x1010 years at z = 0.022 and then decreases to 2.59x109 years at z = 0.1. A piecewise fit of the model lifetimes vs. metallicity was obtained.http://dx.doi.org/10.1051/epjconf/20159303011 |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
Jones E.F. Gore P.M. |
spellingShingle |
Jones E.F. Gore P.M. Modelling the evolution of solar-mass stars with a range of metallicities using MESA EPJ Web of Conferences |
author_facet |
Jones E.F. Gore P.M. |
author_sort |
Jones E.F. |
title |
Modelling the evolution of solar-mass stars with a range of metallicities using MESA |
title_short |
Modelling the evolution of solar-mass stars with a range of metallicities using MESA |
title_full |
Modelling the evolution of solar-mass stars with a range of metallicities using MESA |
title_fullStr |
Modelling the evolution of solar-mass stars with a range of metallicities using MESA |
title_full_unstemmed |
Modelling the evolution of solar-mass stars with a range of metallicities using MESA |
title_sort |
modelling the evolution of solar-mass stars with a range of metallicities using mesa |
publisher |
EDP Sciences |
series |
EPJ Web of Conferences |
issn |
2100-014X |
publishDate |
2015-01-01 |
description |
The nuclides 1,2H, 3,4He, 7Li, 7Be, 8B, 12,13C, 13-15N, 14-18O, 17-19F, 18-22Ne, 22Mg, and 24Mg were used in the code package MESA (Modules for Experiments in Stellar Astrophysics)[Paxton] to model a one-solar-mass star with a range of metallicities, z, from 0 to 0.1. On HR diagrams of each star models luminosity and effective temperature from before zero-age main sequence (pre-ZAMS) to white dwarf, oscillations were noted in the horizontal branch at intervals from z = 0 to 0.0070. At z, = 0, the calculated stellar lifetime is 6.09x109 years. The calculated lifetime of the model stars increases to a maximum of 1.25x1010 years at z = 0.022 and then decreases to 2.59x109 years at z = 0.1. A piecewise fit of the model lifetimes vs. metallicity was obtained. |
url |
http://dx.doi.org/10.1051/epjconf/20159303011 |
work_keys_str_mv |
AT jonesef modellingtheevolutionofsolarmassstarswitharangeofmetallicitiesusingmesa AT gorepm modellingtheevolutionofsolarmassstarswitharangeofmetallicitiesusingmesa |
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