Stellar Populations in Local Group Galaxies (WC13): Cycle 4 and Future-Cycle Continuation

Details Stellar Populations in Local Group Galaxies (WC13): Cycle 4 and Future-Cycle Continuation Stellar Populations in Local Group Galaxies (WC13): Cycle 4 and Future-Cycle Continuation

Jul 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994hst..prop.5113w&link_type=abstract

HST Proposal ID #5113

Physics

Hst Proposal Id #5113

Scientific paper

The goal of this WF/PC project is to extend our knowledge of the stellar population in arms, disks, and bulges of the nearest star-producing galaxies. In M31 our targets include one giant HII region (NGC206), two arm samples (Baade Fields 3 and 4), two disk samples adjacent to those arms, and one position in the bulge. In M33 our targets include one giant HII region (NGC604) and one arm field (cluster C27). Deep U, V, I frames will be used to construct color-magnitude and color-color diagrams, and to derive age, metallicity, reddening, and luminosity functions.

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