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A photometric study of Be stars located in the seismology fields of COROT

Author
GUTIERREZ-SOTO, J1 2 ; FABREGAT, J1 2 ; SUSO, J3 ; LANZARA, M3 ; GARRIDO, R4 ; HUBERT, A.-M2 ; FLOQUET, M2
[1] Observatorio Astronómico, Universidad de Valencia, edificio Institutos de Investigación, polígono la Coma, 46980 Paterna, Valencia, Spain
[2] GEPI, Observatoire de Paris, CNRS, Université Paris Diderot; place Jules Janssen, 92195 Meudon, France
[3] GACE-ICMUV, edificio Institutos de Investigación, polígono la Coma, 46980 Paterna, Valencia, Spain
[4] Instituto de Astrofísica de Andalucía (CSIC), calle Camino Bajo de Huétor, 24, 18008, Granada, Spain
Source

Astronomy and astrophysics (Berlin. Print). 2007, Vol 476, Num 2, pp 927-933, 7 p ; ref : 1/2 p

CODEN
AAEJAF
ISSN
0004-6361
Scientific domain
Astronomy earth cosmic environment
Publisher
EDP Sciences, Les Ulis
Publication country
France
Document type
Article
Language
English
Author keyword
stars: emission-line, Be stars: oscillations (including pulsations) stars: statistics techniques: photometric
Keyword (fr)
Courbe lumière Etoile B Etoile premier type Etoile raie émission Etoile rotation Etoile type avancé Observation photométrique Pulsation non radiale Pulsation stellaire Série temporelle Variation court terme
Keyword (en)
Light curves B stars Early type stars Emission line stars Rotating star Late type stars Photometric observation Non radial pulsation Stellar pulsations Time series Short term variation
Keyword (es)
Estrella rotación Observación fotométrica Pulsación no radial Variación corto plazo
Classification
Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy

Discipline
Astronomy
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
19868909

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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