Boron abundances in B-type stars: A test of rotational depletion during main-sequence evolution

Astrophysical Journal

Volumn 565, Issue 1 I, 2002, Pages 571-586

  Venn, K A ^a,g   Brooks, A M ^a   Lambert, David L ^b   Lemke, M ^c   Langer, N ^d   Lennon, D J ^e   Keenan, F P ^f  

^a MACALESTER COLLEGE   (United States)

^b UNIVERSITY OF TEXAS AT AUSTIN   (United States)

^c Dr Remeis Sternwarte Bamberg   (Germany)

^d UTRECHT UNIVERSITY   (Netherlands)

^e ISAAC NEWTON GROUP OF TELESCOPES   (Spain)

^f QUEEN'S UNIVERSITY BELFAST   (United Kingdom)

^g University of Minnesota   (United States)

Author keywords

Stars: abundances; Stars: evolution; Stars: rotation

Indexed keywords

EID: 0012233433     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/324435     Document Type: Article

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