Hot massive stars in M33: HST UV spectroscopy and photometry

Details Hot massive stars in M33: HST UV spectroscopy and photometry Hot massive stars in M33: HST UV spectroscopy and photometry

May 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997aipc..408..135b&link_type=abstract

The ultraviolet universe at low and high redshift. AIP Conference Proceedings, Volume 408, pp. 135-138 (1997).

Computer Science

Spiral Galaxies, Stellar Content And Populations, Radii, Morphology And Overall Structure, Ultraviolet, Stellar Characteristics And Properties

Scientific paper

HST is used to study massive star populations in galaxies of the Local
Group beyond the Magellanic Clouds (M31, M33, NGC6822). The purpose is
to compare massive star parameters in parent galaxies with different
metallicities and star formation histories. Some results for hot stars
in M33 are described here.

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