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Département d'Astronomie Département d'Astronomie

Database

Welcome on the database for stellar models.

You’ll find below the links to the stellar evolution tracks computed by our group.

These tracks come from two distinct codes:

All the tracks referenced below are available in our

 

interactive tools webpage

 

Tracks, isochrones, and spectra can also be downloaded through the link in the references. A description of the electronic tables provided can be found here

  • GRIDS OF STELLAR MODELS WITH ROTATION [ ] — [ ]
    • I. Models from 0.8 to 120 M⊙ at solar metallicity (Z = 0.014)
      Ekström 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⊙ at a metallicity Z = 0.002
      Georgy et al. (2013) A&A 558, A103 [ - - ]
    • IV. Models from 1.7 to 120 M⊙ at a metallicity Z = 0.0004
      Groh et al. (2019) A&A 627, A24 [ - - ]
    • V. Models from 1.7 to 120 M⊙ at zero metallicity
      Murphy et al. (2021) MNRAS 501, 2745 [ - - ]
    • VI. Models from 0.8 to 120 M⊙ at a metallicity Z = 0.006
      Eggenberger et al. (2021) A&A 652, 137 [ - - ]
    • VII: Models from 0.8 to 300 M⊙ at supersolar metallicity (Z = 0.020)
      Yusof et al. (2022) MNRAS 511, 2814 [ - - ]
  • POPULATIONS OF ROTATING STARS [ ]
    • 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 et al. (2013) A&A 553, A24 [ - - ]
    • II. Rapid rotators and their link to Be-type stars
      Granada et al. (2013) A&A 553, A25 [ - - ]
    • III. SYCLIST, the new Geneva Population Synthesis code
      Georgy et al. (2014) A&A 566, A21 [ - - ]
  • GRIDS OF STELLAR MODELS WITH BINARY INTERACTIONS []
    • I. Models from 10 to 60 M⊙ of binary systems with tidal interactions at solar metallicity (Z = 0.014)
      Sciarini et al. (2025) A&A [ A&A - ADS - arXiv]
  • 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⊙
      Mowlavi et al. (2012) A&A 541, A41 [ - - ]
  • Fundamental properties of core-collapse supernova and GRB progenitors: predicting the look of massive stars before death [ ]
    Groh et al. (2013) A&A 558, A301 [ - - ]
  • THE EVOLUTION OF MASSIVE STARS AND THEIR SPECTRA [ ]
    • I. A non-rotating 60 M⊙ star from the ZAMS to the pre-SN stage
      Groh et al. (2014) A&A 564, A30 [ - - ]
  • Non-standard s-process in massive rotating stars. Yields of 10-150 M☉ models at Z = 10-3 [ ]
    Choplin et al. (2018) A&A 618, A133 [ - - ]
  • Stellar models and isochrones from low-mass to massive stars including pre-main sequence phase with accretion [ ] - [ ]
    Haemmerlé et al. (2019) A&A 624, A137 [ - - ]
  • Revisiting Kepler-444. II. Rotational, orbital and high-energy fluxes evolution of the system[ ]
    Pezzotti et al. (2021) A&A (in press) [ ]

All the articles related to the STAREVOL code can be retrieved .

The tracks corresponding to the following articles can be downloaded:

  • 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 [ - - ]

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  • 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 [ - - ]

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  • 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 &amp. al. (2017) A&A 604, A113, [ - - - ]