Abstract
ABSTRACT High-resolution X-ray observations of Mrk 279 with the Einstein Observatory clearly establish it as the optical counterpart of the X-ray source 3A1349 +700 and resolve the ambiguity introduced by the observations of Dower et al. (1980). Mrk 279 exhibits X-ray and optical properties typical of other Seyfert 1 galaxies.
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Schedule a callMore From: Publications of the Astronomical Society of the Pacific
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