NGC6822: short period variable stars, stellar population and distance scale

Simple item page
dc.creatorBaldacci, L.
dc.creatorRizzi, L.
dc.creatorClementini, G.
dc.creatorHeld, E. V.
dc.creator.
dc.date2003-10-20
dc.date.accessioned2026-07-07T02:10:38Z
dc.date.available2026-07-07T02:10:38Z
dc.descriptionResults are presented on a study of the short period variable stars in the dwarf irregular galaxy NGC6822. We observed an almost uniformely populated classical instability strip from the Horizontal Branch up to the Classical Cepheids region. The main goal we achieved from the analysis of the faint sample is the first detection of RR Lyrae stars in this galaxy.
dc.description4 pages, 2 figures, Proceedings of the IAU Colloq. 193, "Variable Stars in the Local Group", ed. D. W. Kurtz & K. R. Pollard., ASP Conf. Ser., in press
dc.identifierhttps://arxiv.org/abs/astro-ph/0310540
dc.identifierhttp://arxiv.org/abs/astro-ph/0310540
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/6799
dc.subjectAstrophysics
dc.titleNGC6822: short period variable stars, stellar population and distance scale
dc.typetext

Files

Collections

arXiv