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EVOLUTIONARY TRACKS of 1.6 to 20 MSun stellar models with new OPAL opacities
J. Daszyńska-Daszkiewicz, P. Walczak, Instytut Astronomiczny Uniwersytetu Wrocławskiego
The evolutionary tracks have been calculated for stellar models from 1.8 up to 12 solar masses in the MS and early post-MS evolutionary stages. The results were obtained for Z=0.020 and reffered as A04 (Asplund et al. 2005).
Pobierz:
- OPAL, AGSS09, AC=0, AO=0.1, V=0, X=0.75, Z=0.008
- OPAL, AGSS09, AC=0, AO=0.1, V=0, X=0.75, Z=0.015
- OPAL, AGSS09, AC=0, AO=0.1, V=0, X=0.75, Z=0.01
- OPAL, AGSS09, AC=0, AO=0.1, V=0, X=0.75, Z=0.02
- OPAL, AGSS09, AC=0, AO=0.1, V=0, X=0.7, Z=0.007
- OPAL, AGSS09, AC=0, AO=0.1, V=0, X=0.7, Z=0.008
- OPAL, AGSS09, AC=0, AO=0.1, V=0, X=0.7, Z=0.015
- OPAL, AGSS09, AC=0, AO=0.1, V=0, X=0.7, Z=0.01
- OPAL, AGSS09, AC=0, AO=0.1, V=0, X=0.7, Z=0.02
- OPAL, AGSS09, AC=0, AO=0.1, V=100, X=0.75, Z=0.008
- OPAL, AGSS09, AC=0, AO=0.1, V=100, X=0.75, Z=0.015
- OPAL, AGSS09, AC=0, AO=0.1, V=100, X=0.75, Z=0.01
- OPAL, AGSS09, AC=0, AO=0.1, V=100, X=0.75, Z=0.02
- OPAL, AGSS09, AC=0, AO=0.1, V=100, X=0.7, Z=0.007
- OPAL, AGSS09, AC=0, AO=0.1, V=100, X=0.7, Z=0.008
- OPAL, AGSS09, AC=0, AO=0.1, V=100, X=0.7, Z=0.015
- OPAL, AGSS09, AC=0, AO=0.1, V=100, X=0.7, Z=0.01
- OPAL, AGSS09, AC=0, AO=0.1, V=100, X=0.7, Z=0.02
- OPAL, AGSS09, AC=0, AO=0.1, V=200, X=0.75, Z=0.008
- OPAL, AGSS09, AC=0, AO=0.1, V=200, X=0.75, Z=0.015
- OPAL, AGSS09, AC=0, AO=0.1, V=200, X=0.75, Z=0.01
- OPAL, AGSS09, AC=0, AO=0.1, V=200, X=0.75, Z=0.02
- OPAL, AGSS09, AC=0, AO=0.1, V=200, X=0.7, Z=0.007
- OPAL, AGSS09, AC=0, AO=0.1, V=200, X=0.7, Z=0.008
- OPAL, AGSS09, AC=0, AO=0.1, V=200, X=0.7, Z=0.015
- OPAL, AGSS09, AC=0, AO=0.1, V=200, X=0.7, Z=0.01
- OPAL, AGSS09, AC=0, AO=0.1, V=200, X=0.7, Z=0.02
- OPAL, AGSS09, AC=0, AO=0.2, V=0, X=0.75, Z=0.008
- OPAL, AGSS09, AC=0, AO=0.2, V=0, X=0.75, Z=0.015
- OPAL, AGSS09, AC=0, AO=0.2, V=0, X=0.75, Z=0.01
- OPAL, AGSS09, AC=0, AO=0.2, V=0, X=0.75, Z=0.02
- OPAL, AGSS09, AC=0, AO=0.2, V=0, X=0.7, Z=0.007
- OPAL, AGSS09, AC=0, AO=0.2, V=0, X=0.7, Z=0.008
- OPAL, AGSS09, AC=0, AO=0.2, V=0, X=0.7, Z=0.01
- OPAL, AGSS09, AC=0, AO=0.2, V=0, X=0.7, Z=0.02
- OPAL, AGSS09, AC=0, AO=0.2, V=0, X=0.7, Z=0.15
- OPAL, AGSS09, AC=0, AO=0.2, V=100, X=0.75, Z=0.008
- OPAL, AGSS09, AC=0, AO=0.2, V=100, X=0.75, Z=0.015
- OPAL, AGSS09, AC=0, AO=0.2, V=100, X=0.75, Z=0.01
- OPAL, AGSS09, AC=0, AO=0.2, V=100, X=0.75, Z=0.02
- OPAL, AGSS09, AC=0, AO=0.2, V=100, X=0.7, Z=0.007
- OPAL, AGSS09, AC=0, AO=0.2, V=100, X=0.7, Z=0.008
- OPAL, AGSS09, AC=0, AO=0.2, V=100, X=0.7, Z=0.015
- OPAL, AGSS09, AC=0, AO=0.2, V=100, X=0.7, Z=0.01
- OPAL, AGSS09, AC=0, AO=0.2, V=100, X=0.7, Z=0.02
- OPAL, AGSS09, AC=0, AO=0.2, V=200, X=0.07, Z=0.02
- OPAL, AGSS09, AC=0, AO=0.2, V=200, X=0.75, Z=0.008
- OPAL, AGSS09, AC=0, AO=0.2, V=200, X=0.75, Z=0.015
- OPAL, AGSS09, AC=0, AO=0.2, V=200, X=0.75, Z=0.01
- OPAL, AGSS09, AC=0, AO=0.2, V=200, X=0.75, Z=0.02
- OPAL, AGSS09, AC=0, AO=0.2, V=200, X=0.7, Z=0.007
- OPAL, AGSS09, AC=0, AO=0.2, V=200, X=0.7, Z=0.008
- OPAL, AGSS09, AC=0, AO=0.2, V=200, X=0.7, Z=0.015
- OPAL, AGSS09, AC=0, AO=0.2, V=200, X=0.7, Z=0.01
- OPAL, AGSS09, AC=0, AO=0, V=0, X=0.75, Z=0.008
- OPAL, AGSS09, AC=0, AO=0, V=0, X=0.75, Z=0.015
- OPAL, AGSS09, AC=0, AO=0, V=0, X=0.75, Z=0.01
- OPAL, AGSS09, AC=0, AO=0, V=0, X=0.75, Z=0.02
- OPAL, AGSS09, AC=0, AO=0, V=0, X=0.7, Z=0.007
- OPAL, AGSS09, AC=0, AO=0, V=0, X=0.7, Z=0.015
- OPAL, AGSS09, AC=0, AO=0, V=0, X=0.7, Z=0.01
- OPAL, AGSS09, AC=0, AO=0, V=0, X=0.7, Z=0.02
- OPAL, AGSS09, AC=0, AO=0, V=100, X=0.75, Z=0.008
- OPAL, AGSS09, AC=0, AO=0, V=100, X=0.75, Z=0.015
- OPAL, AGSS09, AC=0, AO=0, V=100, X=0.75, Z=0.01
- OPAL, AGSS09, AC=0, AO=0, V=100, X=0.75, Z=0.02
- OPAL, AGSS09, AC=0, AO=0, V=100, X=0.7, Z=0.007
- OPAL, AGSS09, AC=0, AO=0, V=100, X=0.7, Z=0.008
- OPAL, AGSS09, AC=0, AO=0, V=100, X=0.7, Z=0.015
- OPAL, AGSS09, AC=0, AO=0, V=100, X=0.7, Z=0.01
- OPAL, AGSS09, AC=0, AO=0, V=100, X=0.7, Z=0.02
- OPAL, AGSS09, AC=0, AO=0, V=200, X=0.75, Z=0.008
- OPAL, AGSS09, AC=0, AO=0, V=200, X=0.75, Z=0.015
- OPAL, AGSS09, AC=0, AO=0, V=200, X=0.75, Z=0.01
- OPAL, AGSS09, AC=0, AO=0, V=200, X=0.75, Z=0.02
- OPAL, AGSS09, AC=0, AO=0, V=200, X=0.7, Z=0.007
- OPAL, AGSS09, AC=0, AO=0, V=200, X=0.7, Z=0.008
- OPAL, AGSS09, AC=0, AO=0, V=200, X=0.7, Z=0.015
- OPAL, AGSS09, AC=0, AO=0, V=200, X=0.7, Z=0.01
- OPAL, AGSS09, AC=0, AO=0, V=200, X=0.7, Z=0.02
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- wszystko
| OPAL | – | OPAL opacities (Iglesias, C.A., Rogers, F.J., 1996, ApJ 464, 943) |
| AGSS09 | – | Chemical Composition (Asplund, M., Grevesse, N., Sauval, A.J., Scott, P., 2009, ARA&A 47, 481A) |
| X | – | hydrogen abundance |
| Z | – | heavy element abundance |
| AC | – | MLT parameter (mixing-length theory); AC = alpha convective = lconv/Hp, where lconv - mixing length, Hp - local pressure scale height |
| AO | – | convective overshooting parameter; AO = alpha overshooting = dover/Hp, where dover - convective overshooting |
| V | – | initial equatorial rotational velocity [km/s] |
BIBLIOGRAFIA:
- Iglesias, C.A., Rogers, F.J., 1996, ApJ 464, 943
- Asplund, M., Grevesse, N., Sauval, A.J., Scott, P., 2009, ARA&A 47, 481A
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