Base de données
Bienvenue sur notre base de données de modèles stellaires.
Vous trouverez ci-dessous les liens vers les tracés évolutifs stellaires calculés par notre groupe.
Ces tracés sont issus de deux codes distincts :
Tous les tracés évolutifs référencés ci-dessous sont disponible sur notre
Les tracés et les isochrones peuvent aussi être téléchargés grâce au lien donné dans les références. Une description des tables électroniques produites peut être trouvée ici.
- GRIDS OF STELLAR MODELS WITH ROTATION [ tracés ] — [ isochrones ]
- I. Models from 0.8 to 120 M⊙ at solar metallicity (Z = 0.014)
Ekström et al. (2012) A&A 537, A146 [ A&A - ADS - arXiv ] - II. Wolf-Rayet populations and supernovae/GRB progenitors at Z = 0.014
Georgy et al. (2012) A&A 542, A29 [ A&A - ADS - arXiv ] - III. Models from 0.8 to 120 M⊙ at a metallicity Z = 0.002
Georgy et al. (2013) A&A 558, A103 [ A&A - ADS - arXiv ] - IV. Models from 1.7 to 120 M⊙ at a metallicity Z = 0.0004
Groh et al. (2019) A&A 627, A24 [ A&A - ADS - arXiv ] - V. Models from 1.7 to 120 M⊙ at zero metallicity
Murphy et al. (2021) MNRAS 501, 2745 [ MNRAS - ADS - arXiv ] - VI. Models from 0.8 to 120 M⊙ at a metallicity Z = 0.006
Eggenberger et al. (2021) A&A 652, A137 [ A&A - ADS ] - VII: Models from 0.8 to 300 M⊙ at supersolar metallicity (Z = 0.020)
Yusof et al. (2022) MNRAS 511, 2814 [ MNRAS - ADS - arXiv ]
- I. Models from 0.8 to 120 M⊙ at solar metallicity (Z = 0.014)
- STELLAR MASS AND AGE DETERMINATIONS [ tracés ]
- POPULATIONS OF ROTATING STARS [ tracés ]
- I. Models from 1.7 to 15 M⊙ at Z = 0.014, 0.006, and 0.002 with Ω/Ωcrit between 0 and 1
Georgy & al. (2013) A&A 553, A24 [ A&A - ADS - arXiv ] - II. Rapid rotators and their link to Be-type stars
Granada & al. (2013) A&A 553, A25 [ A&A - ADS - arXiv ] - III. SYCLIST, the new Geneva Population Synthesis code
Georgy & al. (2014) A&A 566, A21 [ A&A - ADS - arXiv ]
- I. Models from 1.7 to 15 M⊙ at Z = 0.014, 0.006, and 0.002 with Ω/Ωcrit between 0 and 1
- Fundamental properties of core-collapse supernova and GRB progenitors: predicting the look of massive stars before death [ spectres ]
Groh & al. (2013) A&A 558, A301 [ A&A - ADS - arXiv ]
- THE EVOLUTION OF MASSIVE STARS AND THEIR SPECTRA [ spectres ]
- Non-standard s-process in massive rotating stars. Yields of 10-150 M☉ models at Z = 10-3 [ yields ]
Choplin & al. (2018)A&A 618, A133 [ A&A - ADS - arXiv ]
- Stellar models and isochrones from low-mass to massive stars including pre-main sequence phase with accretion [ tracés ] - [ isochrones ]
Haemmerlé & al. (2019) A&A 624, A137 [A&A - ADS - arXiv ]
Tous les articles reliés au code STAREVOL se trouvent ici.
Les tracés correspondants aux articles suivants peuvent être téléchargés :
- THERMOHALINE INSTABILITY AND ROTATION-INDUCED MIXING [ tracés ]
- EVOLUTION OF LONG-LIVED GLOBULAR CLUSTER STARS [ tracés ]
- Tidal dissipation in rotating low-mass stars and implications for the orbital evolution of close-in planets