Astronomy and Astrophysics – Astronomy
Scientific paper
Jun 1988
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988esasp.281a.417s&link_type=abstract
In ESA, A Decade of UV Astronomy with the IUE Satellite, Volume 1 p 417-420 (SEE N89-10682 01-89)
Astronomy and Astrophysics
Astronomy
1
Iue, Magellanic Clouds, Spaceborne Astronomy, Stellar Spectra, Supergiant Stars, Ultraviolet Astronomy, Emission Spectra, Optical Properties, Ultraviolet Spectra
Scientific paper
The Henize-Carlson sample of galactic massive supergiants, and a comparison between the Galactic and LMC samples are discussed. Several of the stars, notably He3-395 and S 127/LMC, have very similar shell characteristics. There appears to be little difference, other than luminosity, between the LMC and Galactic samples. One star, He3-1482, was detected with the Very Large Array at 6 cm. The UV data is combined with IRAS and optical information.
Bopp Bernard William
Brown David N.
Robinson Craig Richard
Sanduleak Nicholas
Shore Steve N.
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