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

Astronomy and Astrophysics

Volumn 476, Issue 2, 2007, Pages 927-933

  Gutierrez Soto J ^a,b   Fabregat, J ^a,b   Suso, J ^a   Lanzara, M ^a   Garrido, R ^c   Hubert, A M ^b   Floquet, M ^b  

^a UNIVERSITY OF VALENCIA   (Spain)

^b UNIVERSITÉ PARIS DIDEROT   (France)

^c INSTITUTO DE ASTROFÍSICA DE ANDALUCÍA CSIC   (Spain)

Author keywords

Stars: emission line, Be; Stars: oscillations (including pulsations); Stars: statistics; Techniques: photometric

Indexed keywords

LEAST SQUARES APPROXIMATIONS; PHOTOMETRY; SATELLITES; SEISMOLOGY;

LIGHT CURVES; PULSATIONAL PROPERTIES; SHORT-TERM VARIABILITY;

STARS;

EID: 38049110298     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20078252     Document Type: Article

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