Stellar Winds in M31, M33

Details Stellar Winds in M31, M33 Stellar Winds in M31, M33

Jul 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991hst..prop.1150h&link_type=abstract

HST Proposal ID #1150

Computer Science

Hst Proposal Id #1150

Scientific paper

We will obtain UV spectra of OB supergiant stars in M33 AND M31 to study stellar wind phenomena (resonance line profiles and velocities, stellar effective temperatures). We will also derive approximate UV extinction curves for these galaxies. These observations relate to global comparisons between galaxies of different types. WFC UV grating images are requested in parallel to study the OB star population and extinction in these galaxies.

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