SSP models for star clusters in tidal fields (Anders+, 2009)

Details SSP models for star clusters in tidal fields (Anders+, 2009) SSP models for star clusters in tidal fields (Anders+, 2009)

Jun 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009ycat..35020817a&link_type=abstract

VizieR On-line Data Catalog: J/A+A/502/817. Originally published in: 2009A&A...502..817A

Physics

Models: Evolutionary, Photometry

Scientific paper

Simple Stellar Population (SSP) models for star clusters in tidal fields, based on the GALEV code (GALEV group webpage )
All models are calculated for a universal Kroupa (2001) IMF and for Padova isochrones (Isochrones from the Padova group, as described in Bertelli et al., 1994A&AS..106..275B, Cat. and references therein; with an update on TP-AGB phase 1999).
Data are available at http://www.phys.uu.nl/~anders/data/SSP_varMF The site is going to be updated regularly.
(4 data files).

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