UV-bright stars in globular clusters

Details UV-bright stars in globular clusters UV-bright stars in globular clusters

Jan 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994stin...9424666l&link_type=abstract

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Astronomy and Astrophysics

Astronomy

Globular Clusters, Hot Stars, Subdwarf Stars, Ultraviolet Astronomy, Ultraviolet Telescopes, Astronomical Models, Imaging Techniques, Spaceborne Astronomy, Ultraviolet Spectrometers

Scientific paper

This paper highlights globular cluster studies with Ultraviolet Imaging Telescope (UIT) in three areas: the discrepancy between observed ultraviolet HB magnitudes and predictions of theoretical HB models; the discovery of two hot subdwarfs in NGC 1851, a globular not previously known to contain such stars; and spectroscopic follow up of newly identified UV-bright stars in M79 and w Cen. I also present results of a recent observation of NGC 6397 with the Voyager ultraviolet spectrometer.

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