Surface-brightness fluctuations in stellar populations. IAC-star models for the optical and near-IR wavelengths
Aims.A new theoretical calibration of surface-brightness fluctuations (SBF) for single age, single metallicity stellar populations is presented for the optical and near-IR broad-band filters, as well as for the HST WFPC2 and ACS filters. Methods: .The IAC-star code is used. Two Padua and the Teramo stellar evolution libraries have been considered
Marín-Franch, A. et al.
Fecha de publicación:
5
2006