Most detects g-modes in the late-type Be star β canis minoris (B8 Ve)

Astrophysical Journal

Volumn 654, Issue 1 I, 2007, Pages 544-550

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

^a TOHOKU UNIVERSITY   (Japan)

^b UNIVERSITY OF BRITISH COLUMBIA   (Canada)

^c Universität Wien ^*  (Canada)

^d UNIVERSITY OF VIENNA   (Austria)

^e SAINT MARY S UNIVERSITY   (Canada)

^f UNIVERSITÉ DE MONTRÉAL   (Canada)

^g Observatoire du Mont Megantic   (Canada)

^h UNIVERSITY OF TORONTO   (Canada)

ⁱ HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

Author keywords

Stars: early type; Stars: emission line, Be; Stars: individual ( Canis Minoris); Stars: oscillations; Stars: rotation

Indexed keywords

EID: 33846502112     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/509315     Document Type: Article

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