New evolutionary models for pre-main sequence and main sequence low-mass stars down to the hydrogen-burning limit (2015)
Attributed to:
From Molecular Clouds to Exoplanets
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.1051/0004-6361/201425481
Publication URI: http://dx.doi.org/10.1051/0004-6361/201425481
Type: Journal Article/Review
Parent Publication: Astronomy & Astrophysics