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1994ApJS...90..467D - Astrophys. J., Suppl. Ser., 90, 467-500 (1994/January-0)
New pre-main-sequence tracks for M < 2.5 M as tests of opacities and convection model.
D'ANTONA F. and MAZZITELLI I.
Abstract (from CDS):
Abstract Copyright: ∼
Journal keyword(s): Stars: Pre-Main-Sequence - Convection - Atomic Processes - Stars: Abundances - Stars: Interiors
Simbad objects: 0
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