EXOSAT deep exposure of the LMC X-4 region

Details EXOSAT deep exposure of the LMC X-4 region EXOSAT deep exposure of the LMC X-4 region

Nov 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989esasp.296..573p&link_type=abstract

In ESA, The 23rd ESLAB Symposium on Two Topics in X Ray Astronomy. Volume 1: X Ray Binaries p 573-577 (SEE N90-25711 19-89)

Astronomy and Astrophysics

Astronomy

5

Exosat Satellite, Magellanic Clouds, Star Clusters, Stellar Spectra, X Ray Astronomy, X Ray Sources, Emission Spectra, Star Distribution, Supernova Remnants, Ultraviolet Radiation, Ultraviolet Spectra, Variability, X Ray Telescopes

Scientific paper

EXOSAT observations of the LMC X-4 region, obtained with the low energy X ray telescope and cylindrical mirror analyzer and 3000A Lexan filter are presented. They are combined into one image. LMC X-4 and all the other Einstein sources in the field (the supernova remnants N49 and N63A and the Me star LHG57) are detected in the EXOSAT image and in addition the X ray source EXO 053109-6609.2. This EXOSAT LMC (Large Magellanic Cloud) transient is only visible during 1983. The star HD 37935, the emission nebulae N55 and N55A, a stellar association near N62A, the star cluster NGC2003 are not detected due to UV radiation leaking through the filter.

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