Base de donn茅es
Bienvenue sur notre base de donn茅es de mod猫les stellaires.
Vous trouverez ci-dessous les liens vers les 迟谤补肠茅蝉 茅volutifs stellaires calcul茅s par notre groupe.
Ces 迟谤补肠茅蝉 sont issus de deux codes distincts听:
Tous les 迟谤补肠茅蝉 茅volutifs r茅f茅renc茅s ci-dessous sont disponible sur notre
Les 迟谤补肠茅蝉 et les isochrones peuvent aussi 锚tre t茅l茅charg茅s gr芒ce au lien donn茅 dans les r茅f茅rences. Une description des tables 茅lectroniques produites peut 锚tre trouv茅e ici.
- GRIDS OF STELLAR MODELS WITH ROTATION [ ] 鈥� [ ]
- I. Models from 0.8 to 120 M鈯� at solar metallicity (Z = 0.014)
Ekstr枚m et al. (2012) A&A 537, A146 [ - - ] - II. Wolf-Rayet populations and supernovae/GRB progenitors at Z = 0.014
Georgy et al. (2012) A&A 542, A29 [ - - ] - III. Models from 0.8 to 120 M鈯� at a metallicity Z = 0.002
Georgy et al. (2013) A&A 558, A103 [ - - ] - IV. Models from 1.7 to 120 M鈯� at a metallicity Z = 0.0004
Groh et al. (2019) A&A 627, A24 [ - - ] - V. Models from 1.7 to 120 M鈯� at zero metallicity
Murphy et al. (2021) MNRAS 501, 2745 [ - - ] - VI. Models from 0.8 to 120 M鈯� at a metallicity Z = 0.006
Eggenberger et al. (2021) A&A 652, A137 [ - ] - VII: Models from 0.8 to 300 M鈯� at supersolar metallicity (Z = 0.020)
Yusof et al. (2022) MNRAS 511, 2814 [ - - ]
- I. Models from 0.8 to 120 M鈯� at solar metallicity (Z = 0.014)
- STELLAR MASS AND AGE DETERMINATIONS [ ]
- I. Grids of stellar models from Z = 0.006 to 0.04 and M = 0.5 to 3.5 M鈯�
Mowlavi & al. (2012) A&A 541, A41 [ - - ]
- I. Grids of stellar models from Z = 0.006 to 0.04 and M = 0.5 to 3.5 M鈯�
- POPULATIONS OF ROTATING STARS [ ]
- I. Models from 1.7 to 15 M鈯� at Z = 0.014, 0.006, and 0.002 with 惟/惟crit between 0 and 1
Georgy & al. (2013) A&A 553, A24 [ - - ] - II. Rapid rotators and their link to Be-type stars
Granada & al. (2013) A&A 553, A25 [ - - ] - III. SYCLIST, the new Geneva Population Synthesis code
Georgy & al. (2014) A&A 566, A21 [ - - ]
- I. Models from 1.7 to 15 M鈯� at Z = 0.014, 0.006, and 0.002 with 惟/惟crit between 0 and 1
- Fundamental properties of core-collapse supernova and GRB progenitors: predicting the look of massive stars before death [ ]
Groh & al. (2013) A&A 558, A301 [ - - ]
- THE EVOLUTION OF MASSIVE STARS AND THEIR SPECTRA [ ]
- I. A non-rotating 60 M鈯� star from the ZAMS to the pre-SN stage
Groh & al. (2014) A&A 564, A30 [ - - ]
- Non-standard s-process in massive rotating stars. Yields of 10-150 M鈽� models at Z = 10-3 [ ]
Choplin & al. (2018)A&A 618, A133 [ - - ]
- Stellar models and isochrones from low-mass to massive stars including pre-main sequence phase with accretion [ ] - [ ]
Haemmerl茅 & al. (2019) A&A 624, A137 [ - - ]
Tous les articles reli茅s au code STAREVOL se trouvent .
Les 迟谤补肠茅蝉 correspondants aux articles suivants peuvent 锚tre t茅l茅charg茅s听:
- THERMOHALINE INSTABILITY AND ROTATION-INDUCED MIXING [ ]
- III. Seismic diagnostics and grid of stellar models from the pre-main sequence up to the AGB for low- and intermediate-mass stars at various metallicities
Lagarde & al. (2012) A&A 543, A108 [ - - ]
- III. Seismic diagnostics and grid of stellar models from the pre-main sequence up to the AGB for low- and intermediate-mass stars at various metallicities
听
- EVOLUTION OF LONG-LIVED GLOBULAR CLUSTER STARS [ ]
- I. Grid of stellar models with helium enhancement at [Fe/H] = -1.75
Chantereau & al. (2015) A&A 578, A117 [ - - ]
- I. Grid of stellar models with helium enhancement at [Fe/H] = -1.75
听
- Tidal dissipation in rotating low-mass stars and implications for the orbital evolution of close-in planets
- I. From the PMS to the RGB at solar metallicity
Gallet & al. (2017) A&A 604, A112 [ - - - ] - II. Effect of stellar metallicity
Bolmont &. al. (2017) A&A 604, A113, [ - - - ]
- I. From the PMS to the RGB at solar metallicity