Surface abundance distribution models of Si, Cr, Mn, Fe, Pr and Nd for the slowly rotating Ap star HD 187474

Astronomy and Astrophysics

Volumn 378, Issue 1, 2001, Pages 153-164

  Strasser, S ^a   Landstreet, J D ^a   Mathys, G ^a  

^a UNIVERSITY OF WESTERN ONTARIO   (Canada)

Author keywords

Stars: abundances; Stars: chemically peculiar; Stars: fundamental properties; Stars: magnetic fields

Indexed keywords

EID: 0035471439     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20011174     Document Type: Article

References (30)