NGC 4214: Cluster Properties Derived from Multi-band Photometry

Details NGC 4214: Cluster Properties Derived from Multi-band Photometry NGC 4214: Cluster Properties Derived from Multi-band Photometry

Mar 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009nqsa.conf..157u&link_type=abstract

New Quests in Stellar Astrophysics. II. Ultraviolet Properties of Evolved Stellar Populations, Proceedings of the International

Astronomy and Astrophysics

Astrophysics

Scientific paper

We present the results of a detailed UV-optical study of some of the stellar clusters in the nearby dwarf starburst galaxy NGC 4214 using multifilter HST/WFPC2+STIS photometry. The data show the existence of both young and old stellar populations that can be resolved at the distance of NGC 4214 (2.94 Mpc). We detected a number of massive clusters and associations with ages between a few and 200 million years and we derived their physical properties by comparing our photometry with low metallicity starburst99 cluster models.

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