EXOSAT and Einstein high resolution images of the Small Magellanic Cloud

Details EXOSAT and Einstein high resolution images of the Small Magellanic Cloud EXOSAT and Einstein high resolution images of the Small Magellanic Cloud

Apr 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985ssrv...40..693j&link_type=abstract

(ESA, ESLAB Symposium on X-Ray Astronomy in the EXOSAT Era, 18th, The Hague, Netherlands, Nov. 5-9, 1984) Space Science Reviews

Astronomy and Astrophysics

Astronomy

10

Exosat Satellite, Image Resolution, Light Curve, Magellanic Clouds, Supernova Remnants, X Ray Sources, Heao 2, X Ray Astronomy, X Ray Binaries

Scientific paper

In order to obtain optical identifications and further information about the X-ray emission of sources discovered in the Einstein IPC survey of the Small Magellanic Cloud (SMC), the authors have used the EXOSAT CMA and Einstein HRI at selected positions. These observations have so far resulted in several identifications (including 4 stellar objects with mv ≡ 14 to ≡21 and a Seyfert galaxy), and the discovery of two new X-ray sources. Medium energy X-rays (2 - 6 keV) have been detected from the brightest SNR in the SMC, 1E0102.2-7219. The authors present an initial report of these results.

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