Abstract
We present some results of an observational and theoretical study on unresolved stellar
systems based on the Surface Brightness Fluctuations (SBF) technique. It is shown that SBF
magnitudes are a valuable tracer of stellar population properties, and a reliable distance indicator.
SBF magnitudes, SBF-colors, and SBF-gradients can help to constrain within relatively narrow
limits the metallicity and age of the dominant stellar component in distant stellar systems, especially
if coupled with other spectro-photometric indicators.
Original language | Undefined/Unknown |
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Title of host publication | Probing stellar populations out to the distant universe: Cefalu 2008, proceedings of the international conference |
Editors | G. Giobbi |
Publisher | American Institute of Physics |
Pages | 35-38 |
Number of pages | 4 |
Publication status | Published - 7 Sept 2008 |