Horizontal branch stars, and galactic and magellanic cloud globular clusters

Details Horizontal branch stars, and galactic and magellanic cloud globular clusters Horizontal branch stars, and galactic and magellanic cloud globular clusters

Jun 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981nascp2171..527d&link_type=abstract

In NASA. Goddard Space Flight Center The Universe at Ultraviolet Wavelengths: The First Two Yrs. of Intern. Ultraviolet Explo

Astronomy and Astrophysics

Astronomy

1

Energy Distribution, Galactic Clusters, Globular Clusters, Magellanic Clouds, Stellar Atmospheres, Stellar Models, Stellar Temperature, Brightness Temperature, Iue, Spaceborne Astronomy, Ultraviolet Astronomy

Scientific paper

Seven blue horizontal branch stars in the field were observed and a few HB stars were isolated in globular clusters. Energy distributions are compared to assess possible differences and also used in comparison with model atmospheres. Observed energy distributions of HB stars in NGC 6397 are used to estimate the total number of HB stars which produced the integrated fluxes as observed by ANS. Preliminary results are given for colors of globular clusters observed in the Magellanic Clouds and for their extent, based on the Washburn IUE extraction.

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