IUE and optical observations of X-ray sources in the Large Margellanic Cloud (LMC)

Details IUE and optical observations of X-ray sources in the Large Margellanic Cloud (LMC) IUE and optical observations of X-ray sources in the Large Margellanic Cloud (LMC)

Jun 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988esasp.281a.145b&link_type=abstract

In ESA, A Decade of UV Astronomy with the IUE Satellite, Volume 1 p 145-148 (SEE N89-10682 01-89)

Astronomy and Astrophysics

Astronomy

9

Iue, Magellanic Clouds, Spaceborne Astronomy, Ultraviolet Astronomy, X Ray Sources, Space Observations (From Earth), Spectrum Analysis, Stellar Luminosity, Stellar Temperature

Scientific paper

The optical counterparts of LMC X-6 (star Wo564) and of LHG-8 (HV5542) were observed with IUE and with optical instruments on the ground. The analysis of the UV spectral features and continuum flux, from which the values of the effective temperature and bolometric luminosity of the stars are derived, is outlined. Ultraviolet and optical observations of the source LHG-83, obtained over a 3 yr period, are also analyzed.

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