Models from Baraffe, Homeier, Allard, Chabrier 2015, A&A,577, 42
"New evolutionary models for pre-main sequence and main sequence low-mass stars down to the hydrogen-burning limit"

NOTE: Isochrones in different filters will be regularly added on this site.

The file BHAC15_tracks+structure include tracks and some information on the internal structure
(mass of the radiative core, gyration radii, central temperature and densities, etc...).


If you have any special request, please contact: i.baraffe@ex.ac.uk

Isabelle Baraffe


Reference to quote: Baraffe et al. 2015

@ARTICLE{2015A&A...577A..42B,
   author = {{Baraffe}, I. and {Homeier}, D. and {Allard}, F. and {Chabrier}, G.
	},
    title = "{New evolutionary models for pre-main sequence and main sequence low-mass stars down to the hydrogen-burning limit}",
  journal = {\aap},
archivePrefix = "arXiv",
   eprint = {1503.04107},
 primaryClass = "astro-ph.SR",
 keywords = {stars: evolution, stars: low-mass, stars: pre-main sequence, Hertzsprung-Russell and C-M diagrams, convection},
     year = 2015,
    month = may,
   volume = 577,
      eid = {A42},
    pages = {A42},
      doi = {10.1051/0004-6361/201425481},
   adsurl = {http://adsabs.harvard.edu/abs/2015A%26A...577A..42B},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}