Diffusion of iron-group elements in the envelopes of HgMn stars

Monthly Notices of the Royal Astronomical Society

Volumn 307, Issue 4, 1999, Pages 1008-1022

  Seaton, M J ^a  

^a UNIVERSITY COLLEGE LONDON   (United Kingdom)

Author keywords

Diffusion; Stars: chemically peculiar

Indexed keywords

BINARY ALLOYS; CHROMIUM; IRON; MANGANESE; MANGANESE ALLOYS; NUMERICAL METHODS; OPACITY; SATELLITES; STARS;

ATMOSPHERIC ABUNDANCE; DIFFUSION OF IRON; IRON GROUP; OPTICAL DEPTH; PRESSURE FORCE; RADIATION PRESSURE; STARS: BE; STARS: CHEMICALLY PECULIAR; STELLAR ENVELOPE; UPPER BOUNDARY;

DIFFUSION;

EID: 0039110033     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.1999.02733.x     Document Type: Article

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