Spatially Resolved mid-UV Spectra of the Centers of Local Group Galaxies

Details Spatially Resolved mid-UV Spectra of the Centers of Local Group Galaxies Spatially Resolved mid-UV Spectra of the Centers of Local Group Galaxies

Jul 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004hst..prop10224s&link_type=abstract

HST Proposal ID #10224

Physics

Hst Proposal Id #10224 Stellar Populations

Scientific paper

We propose to use STIS to collect medium resolution mid-UV and optical spectra from the nuclei of M31, M32 and NGC 205. The observations will provide fundamental constraints to the stellar population models we are currently developing in our Treasury Program {GO-9455, PI Ruth Peterson}. The data will also be useful to constrain the stellar population content in the centers of the target galaxies. Last but not least, they will be crucial templates for studies of distant galaxies, by providing a direct assessment of spectrophotometric evolution in the mid-UV.

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