THE SOLAR NEIGHBORHOOD. XXXVII. THE MASS–LUMINOSITY RELATION FOR MAIN-SEQUENCE M DWARFS
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://stacks.iop.org/1538-3881/152/i=5/a=141/pdf
Reference128 articles.
1. Spherically Symmetric Model Atmospheres for Low‐Mass Pre–Main‐Sequence Stars with Effective Temperatures between 2000 and 6800 K
2. Accurate masses and radii of normal stars
3. New evolutionary models for pre-main sequence and main sequence low-mass stars down to the hydrogen-burning limit
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