Late stages of the evolution of A-type stars on the main sequence: comparison between observed chemical abundances and diffusion models for 8 Am stars of the Praesepe cluster (2007)
Attributed to:
Visitor Support Grant for Theoretical and Observational Astrophysics at Armagh Observatory: 2007-2010
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.1051/0004-6361:20078320
Publication URI: http://dx.doi.org/10.1051/0004-6361:20078320
Type: Journal Article/Review
Parent Publication: Astronomy & Astrophysics
Issue: 2