On the Period-Luminosity-Color Relation of Classical Cepheids

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dc.creatorBono, G.
dc.creatorMarconi, M.
dc.date1998-10-28
dc.date.accessioned2026-07-07T02:28:47Z
dc.date.available2026-07-07T02:28:47Z
dc.descriptionWe present the comparison between theoretical and empirical PL relations in V and I bands for the Large Magellanic Cloud. We found that, within the current intrinsic dispersions, theoretical predictions are in remarkable agreement with observational data. We also discuss the PLC relations in (V,B-V) and (V,V-I) as well as the dependence of distance determinations on uncertainties in colors, in reddening corrections and in metal content.
dc.description6 pages, including 1 postscript figure, IAU Symposium 190
dc.identifierhttps://arxiv.org/abs/astro-ph/9810460
dc.identifierhttp://arxiv.org/abs/astro-ph/9810460
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/13206
dc.subjectAstrophysics
dc.titleOn the Period-Luminosity-Color Relation of Classical Cepheids
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