Pulsational models of BL Her stars

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dc.creatorDi Criscienzo, M.
dc.creatorMarconi, M.
dc.creatorCaputo, F.
dc.creatorCassisi, S.
dc.date2007-12-05
dc.date.accessioned2026-07-07T08:47:26Z
dc.date.available2026-07-07T08:47:26Z
dc.descriptionWe present an updated and homogeneous pulsational scenario for a wide range of stellar parameters typical of BL Her stars i.e., Population II Cepheids with periods shorter than 8 days.
dc.description3 pages, 2 greyscale figures. Proceedings of the workshop "XXI Century challenges for stellar evolution", held in Cefalu' (Sicily, Italy), August 29 - September 2, 2007; S. Cassisi and M. Salaris Eds. To be published in Mem. SAIt Vol. 79 No. 2
dc.identifierhttps://arxiv.org/abs/0712.0701
dc.identifierhttp://arxiv.org/abs/0712.0701
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/143595
dc.subjectAstrophysics
dc.titlePulsational models of BL Her stars
dc.typetext

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