Most detects g-modes in the Be star HD 163868

Astrophysical Journal

Volumn 635, Issue 1 II, 2005, Pages

  Walker, G A H ^a   Kuschnig, R ^b   Matthews, J M ^b   Cameron, C ^b   Saio, H ^c   Lee, U ^c   Kambe, E ^d   Masuda, S ^e   Guenther, D B ^f   Moffat, A F J ^g   Rucinski, S M ^h   Sasselov, D ⁱ   Weiss, W W ^j  

^a University of British Columbia ^*  (Canada)

^b UNIVERSITY OF BRITISH COLUMBIA   (Canada)

^c TOHOKU UNIVERSITY   (Japan)

^d NATIONAL DEFENSE ACADEMY   (Japan)

^e NATIONAL ASTRONOMICAL OBSERVATORY OF JAPAN   (Japan)

^f SAINT MARY S UNIVERSITY   (Canada)

^g UNIVERSITÉ DE MONTRÉAL   (Canada)

^h UNIVERSITY OF TORONTO   (Canada)

ⁱ HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^j UNIVERSITY OF VIENNA   (Austria)

more..

Author keywords

Stars: early type; Stars: emission line, Be Stars: individual (HD 163868); Stars: oscillations; Stars: rotation

Indexed keywords

EID: 30544453937     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/499362     Document Type: Article

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