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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)

First Author: Fossati L

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