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MOST DETECTS SPBe PULSATIONS IN HD 127756 AND HD 217543 : ASTEROSEISMIC ROTATION RATES INDEPENDENT OF v sin i

Author
CAMERON, C1 ; SAIO, H2 ; KUSCHNIG, R3 ; WALKER, G. A. H; MATTHEWS, J. M1 ; GUENTHER, D. B4 ; MOFFAT, A. F. J5 ; RUCINSKI, S. M6 ; SASSELOV, D7 ; WEISS, W. W3
[1] Department of Physics and Astronomy, University of British Columbia, 6224 Agricultural Road, Vancouver, BC V6T 1 Z, Canada
[2] Astronomical Institute, Graduate School of Science, Tohoku University, Sendai, 980-8578, Japan
[3] Institut für Astronomie, Universität Wien, Türkenschanzstrasse 17, 1180 Wien, Austria
[4] Department of Astronomy and Physics, St. Mary's University, Halifax, NS B3H 3C3, Canada
[5] Departement de physique, University de Montréal C.P. 6128, Succursale Centre-Ville, Montreal, QC H3C 3J7, Canada
[6] Department of Astronomy and Astrophysics, David Dunlap Observatory, University Toronto P.O. Box 360, Richmond Hill, ON L4C 4Y6, Canada
[7] Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, United States
Source

The Astrophysical journal. 2008, Vol 685, Num 1, pp 489-507, 19 p ; 1 ; ref : 1/2 p

CODEN
ASJOAB
ISSN
0004-637X
Scientific domain
Astronomy earth cosmic environment
Publisher
University of Chicago Press, Chicago, IL
Publication country
United States
Document type
Article
Language
English
Author keyword
stars: early-type stars: emission-line, Be stars: individual (HD 127756, HD 217543, HD 163868, β CMi) techniques: photometric
Keyword (fr)
Etoile premier type Etoile raie émission Vitesse rotation
Keyword (en)
Early type stars Emission line stars Rotation speed
Keyword (es)
Velocidad rotación
Classification
Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy

Discipline
Astronomy
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
20690760

Sauf mention contraire ci-dessus, le contenu de cette notice bibliographique peut être utilisé dans le cadre d’une licence CC BY 4.0 Inist-CNRS / Unless otherwise stated above, the content of this bibliographic record may be used under a CC BY 4.0 licence by Inist-CNRS / A menos que se haya señalado antes, el contenido de este registro bibliográfico puede ser utilizado al amparo de una licencia CC BY 4.0 Inist-CNRS

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