The supersoft X-ray source RXJ0537.6-7033

Details The supersoft X-ray source RXJ0537.6-7033 The supersoft X-ray source RXJ0537.6-7033

May 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996aas...188.7605o&link_type=abstract

American Astronomical Society, 188th AAS Meeting, #76.05; Bulletin of the American Astronomical Society, Vol. 28, p.952

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Scientific paper

The super-soft X-ray source RXJ0537.6-7033 was observed with the ROSAT PSPC in four occasions in 1992 and 1993 and it was found to be a weak, variable X-ray source with a super--soft spectrum. Optical observations suggest the identification with a variable optical star with the line of He II at 4686 Angstroms \ in emission. The line is redshifted by about 4 Angstroms suggesting the LMC membership. The evidence suggests that it is another "CAL 87--type'' source.

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