Upper Limits of the X-Ray Emission from Supernova 1987A in 2-32-KEV Energy Band in 1987JUNAUG

Details Upper Limits of the X-Ray Emission from Supernova 1987A in 2-32-KEV Energy Band in 1987JUNAUG Upper Limits of the X-Ray Emission from Supernova 1987A in 2-32-KEV Energy Band in 1987JUNAUG

Jul 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988pazh...14..591s&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal, Vol. 14:7, P. 591, 1988

Astronomy and Astrophysics

Astronomy

2

Scientific paper

Before the discovery of the X-ray flux from supernova 1987A in August 1987 the region of the Large Magellanic Cloud was several times observed in 1987 by a number of X-ray instruments. The strongest upper limits on X-ray emission from SN 1987A in 2 - 32 keV energy band in June - August 1987 are obtained by the TTM telescope on the "Mir" - "Kvant" observatory "Roentgen".

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