Stellar Population in the Galactic Bulge (WF/PC-02) Cycle 1

Details Stellar Population in the Galactic Bulge (WF/PC-02) Cycle 1 Stellar Population in the Galactic Bulge (WF/PC-02) Cycle 1

Jul 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991hst..prop.1106w&link_type=abstract

HST Proposal ID #1106

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Hst Proposal Id #1106

Scientific paper

The goal of this WF/PC project is to extend our knowledge of the stellar population in the nuclear bulge of our own Galaxy. During GTO time, our targets include a selected field within Baade's Window (about 4 degrees from the galactic nucleus) and another bulge field about 8 degrees from the nucleus. Stepped exposures with U, V, and I filters will enable us to correct for reddening on a small spatial scale, to extend the color-magnitude diagram several magnitudes, and to investigate the low-mass portion of the luminosity function.

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