Distances and Stellar Population properties using the SBF method

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dc.creatorCantiello, Michele
dc.creatorRaimondo, Gabriella
dc.creatorBrocato, Enzo
dc.creatorBiscardi, Ilaria
dc.date2008-12-11
dc.date.accessioned2026-07-07T12:11:58Z
dc.date.available2026-07-07T12:11:58Z
dc.descriptionWe present some results on the study of stellar population properties and distances of galaxies using the SBF technique. The applications summarized here show that the Surface Brightness Fluctuations (SBF) method is able to i) provide accurate distances of resolved and unresolved stellar systems from ~10 Kpc to ~150 Mpc, and ii) to reliably constrain the physical properties (e.g. age and metallicity) of unresolved stellar systems.
dc.description4 pages
dc.identifierhttps://arxiv.org/abs/0812.2101
dc.identifierhttp://arxiv.org/abs/0812.2101
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/210394
dc.subjectAstrophysics
dc.titleDistances and Stellar Population properties using the SBF method
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