Bulge Stellar Populations in so Galaxies - CYCLE3-HIGH

Details Bulge Stellar Populations in so Galaxies - CYCLE3-HIGH Bulge Stellar Populations in so Galaxies - CYCLE3-HIGH

Jul 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993hst..prop.4843d&link_type=abstract

HST Proposal ID #4843

Physics

Hst Proposal Id #4843

Scientific paper

It is proposed to study the origin of the UV flux in elliptical-type population and to determine the respective contribution from young stars and from hot evolved stars. Two SO galaxies NGC 5102 and NGC 3115, at reasonable distance and with very different gas contents, have been selected. Observations through several filters (especially a far UV filter) will allow to resolve and study the massive stars, if they exist. The UV surface brightness of the unresolved background will be measured and will set constraints on the characteristics of hot evolved stars.

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