Stellar Winds in M31, M33 Cycle 2

Details Stellar Winds in M31, M33 Cycle 2 Stellar Winds in M31, M33 Cycle 2

Jul 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992hst..prop.3954h&link_type=abstract

HST Proposal ID #3954

Computer Science

Hst Proposal Id #3954

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.

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