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

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dc.creatorGutierrez-Soto, J.
dc.creatorFabregat, J.
dc.creatorSuso, J.
dc.creatorHubert, A. M.
dc.creatorFloquet, M.
dc.creatorGarrido, R.
dc.date2003-09-29
dc.date.accessioned2026-07-07T02:09:50Z
dc.date.available2026-07-07T02:09:50Z
dc.descriptionWe 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.
dc.description7 pages, 6 figures, submitted to Communications in Asteroseismology
dc.identifierhttps://arxiv.org/abs/astro-ph/0309773
dc.identifierhttp://arxiv.org/abs/astro-ph/0309773
dc.identifierCommun.Asteros. 143 (2003) 29-35
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/6580
dc.subjectAstrophysics
dc.titlePhotometry of Be Stars in the vicinity of COROT primary targets for asteroseismology
dc.typetext

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