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

Astronomy and Astrophysics

Volumn 476, Issue 2, 2007, Pages 911-925

  Fossati, L ^a   Bagnulo, S ^b   Monier, R ^c   Khan, S A ^d   Kochukhov, O ^e   Landstreet, J ^d   Wade, G ^f   Weiss, W ^a  

^a UNIVERSITY OF VIENNA   (Austria)

^b ARMAGH OBSERVATORY   (United Kingdom)

^c UNIVERSITÉ MONTPELLIER II   (France)

^d UNIVERSITY OF WESTERN ONTARIO   (Canada)

^e UPPSALA UNIVERSITY   (Sweden)

^f ROYAL MILITARY COLLEGE OF CANADA   (Canada)

Author keywords

Stars: abundances; Stars: atmospheres; Stars: chemically peculiar; Stars: fundamental parameters

Indexed keywords

ATMOSPHERIC CHEMISTRY; CLUSTER ANALYSIS; DIFFUSION; MATHEMATICAL MODELS; PHOTOMETRY;

A-TYPE STARS; CHEMICAL PECULIARITIES; DIFFUSION MODELS;

STARS;

EID: 38049110299     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20078320     Document Type: Article

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