Another supersoft X-ray source in the LMC

Details Another supersoft X-ray source in the LMC Another supersoft X-ray source in the LMC

Jan 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994a%26a...281l..61g&link_type=abstract

Astronomy and Astrophysics (ISSN 7004-6361), vol. 281, no. 2, p. L61-L64

Astronomy and Astrophysics

Astronomy

17

Black Body Radiation, Brightness Temperature, Magellanic Clouds, Sky Surveys (Astronomy), Spaceborne Astronomy, White Dwarf Stars, X Ray Astronomy, X Ray Spectra, Astronomical Models, Astronomical Spectroscopy, Mathematical Models, Proportional Counters, Rosat Mission, Stellar Evolution

Scientific paper

We have discovered another supersoft X-ray source with similar
properties as the known supersoft sources in the Large Magellanic Cloud
(LMC). The derived absorption and the lack of a bright optical
counterpart indicate LMC membership. The source exhibits a very low
blackbody temperature of kTbb = 10-30 eV.

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