Photometry of Be Stars in the vicinity of COROT primary targets for asteroseismology

(2) Instituto Ciencia de los Materiales; (3) GEPI; (4) Instituto de Astrofisica de Andalucia); A.M. Hubert (3); J. Fabregat (1); J. Gutierrez-Soto (1); J. Suso (2); M. Floquet (3); Observatoire de Paris-Meudon; R. Garrido (4) ((1) Observatori Astronomic

arxiv: astro-ph/0309773 · v1 · submitted 2003-09-29 · 🌌 astro-ph

Photometry of Be Stars in the vicinity of COROT primary targets for asteroseismology

J. Gutierrez-Soto (1) , J. Fabregat (1) , J. Suso (2) , A.M. Hubert (3) , M. Floquet (3) , R. Garrido (4) ((1) Observatori Astronomic , Universitat de Valencia , (2) Instituto Ciencia de los Materiales

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(3) GEPI Observatoire de Paris-Meudon (4) Instituto de Astrofisica de Andalucia)

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keywords asteroseismologycorotstarstargetsphotometryprimarycloseconsidered

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We present differential photometry of Be stars close to potential COROT primary targets for asteroseismology. Several stars are found to be short period variables. We propose them to be considered as secondary targets in the COROT asteroseismology fields.

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Photometry of Be Stars in the vicinity of COROT primary targets for asteroseismology

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