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29 March 2024
 
  » arxiv » astro-ph/0209573

 Article overview


Surface Brightness Fluctuations: a theoretical point of view
M. Cantiello ; G. Raimondo ; E. Brocato ; M. Capaccioli ;
Date 27 Sep 2002
Subject astro-ph
Affiliation1,2), G. Raimondo (1,3), E. Brocato , M. Capaccioli ( INAF-Osservatorio Astronomico di Collurania, Teramo, Italy, Universita’ degli studi di Salerno, Italy, Universita’ di Roma, La Sapienza, Roma, Italy, INAF-Osservatorio Astronomico di
AbstractWe 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.
Source arXiv, astro-ph/0209573
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