Theoretical models for classical cepheids: V. Multiwavelength relations

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dc.creatorCaputo, F.
dc.creatorMarconi, M.
dc.creatorMusella, I.
dc.date1999-11-23
dc.date.accessioned2026-07-07T13:02:33Z
dc.date.available2026-07-07T13:02:33Z
dc.descriptionFrom a theoretical study based on nonlinear, nonlocal and time-dependent convective pulsating models at varying mass and chemical composition, we present the predicted Period-Luminosity, Period-Color, Color-Color and Period-Luminosity-Color relations in the BVRIJK bands for Classical Cepheids. All the theoretical relations are, in various degrees, metallicity dependent and the comparison with observed data for MC and Galactic Cepheids show a fair agreement which supports the validity of the pulsating models.
dc.description20 pages, 20 postscript figures, accepted for publication on Astronomy and Astrophysics
dc.identifierhttps://arxiv.org/abs/astro-ph/9911441
dc.identifierhttp://arxiv.org/abs/astro-ph/9911441
dc.identifierAstron.Astrophys.354:610-620,2000
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/226487
dc.subjectAstrophysics
dc.titleTheoretical models for classical cepheids: V. Multiwavelength relations
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