Variable stars in Fornax dwarf spheroidal galaxy

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dc.catalogadorpau
dc.contributor.authorGreco, C.
dc.contributor.authorClementini, G.
dc.contributor.authorHeld, E. V.
dc.contributor.authorPoretti, E.
dc.contributor.authorCatelan, Marcio
dc.contributor.authorDell'Arciprete, L.
dc.contributor.authorGullieuszik, M.
dc.contributor.authorMaio, M.
dc.contributor.authorRizzi, L.
dc.contributor.authorSmith, H. A.
dc.contributor.authorPritzl, B. J.
dc.contributor.authorRest, A.
dc.contributor.authorDe Lee, N.
dc.date.accessioned2024-03-05T15:14:41Z
dc.date.available2024-03-05T15:14:41Z
dc.date.issued2005
dc.description.abstractWe present the first results of a variable star search in the field and in the globular clusters of the Fornax dwarf spheroidal galaxy. Variable stars were identified using the Image Subtraction Technique (Alard 2000) on time-series data obtained with the ESO 2.2 m and the Magellan 6.5 m telescopes. The variable star sample includes RR Lyrae stars, Dwarf Cepheids and Anomalous Cepheids. The pulsation properties (namely: periods, light curves, period-amplitude relations and classification in Oosterhoff types) of Fornax variables from the present study are discussed in some detail....
dc.fuente.origenORCID
dc.identifier.doi10.48550/arXiv.astro-ph/0507244
dc.identifier.urihttps://doi.org/10.48550/arXiv.astro-ph/0507244
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/84007
dc.information.autorucInstituto de Astrofísica; Catelan , Marcio; 0000-0001-6003-8877; 1001556
dc.language.isoen
dc.rightsacceso restringido
dc.titleVariable stars in Fornax dwarf spheroidal galaxy
dc.typepreprint
sipa.codpersvinculados1001556
sipa.trazabilidadORCID;2024-01-22
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