Surface Brightness Fluctuations: a theoretical point of view

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dc.creatorCantiello, M.
dc.creatorRaimondo, G.
dc.creatorBrocato, E.
dc.creatorCapaccioli, M.
dc.date2002-09-27
dc.date.accessioned2026-07-07T02:05:26Z
dc.date.available2026-07-07T02:05:26Z
dc.descriptionWe present new theoretical evaluations of optical and near-IR Surface Brightness Fluctuations (SBF) magnitudes for single-burst stellar populations in the age range t=5-15 Gyr and metallicity from $Z_{\sun}/200$ to $2Z_{\sun}$. Our theoretical predictions can be successfully used to derive reliable distance evaluations. They also appear to be a new and valuable tool to trace the properties of unresolved stellar populations.
dc.description2 pages, incl. 1 figure, uses newpasp.sty, to be published in ``New Horizons in Globular Cluster Astronomy'', ASP Conference Series, 2002; Eds.: G. Piotto, G. Meylan, G. Djorgowski and M. Riello, in press
dc.identifierhttps://arxiv.org/abs/astro-ph/0209573
dc.identifierhttp://arxiv.org/abs/astro-ph/0209573
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/5101
dc.subjectAstrophysics
dc.titleSurface Brightness Fluctuations: a theoretical point of view
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