X ray observations of the LMC field by the TTM instrument onboard the KVANT module: November 1988 to June 1989

Details X ray observations of the LMC field by the TTM instrument onboard the KVANT module: November 1988 to June 1989 X ray observations of the LMC field by the TTM instrument onboard the KVANT module: November 1988 to June 1989

Nov 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989esasp.296..633s&link_type=abstract

In ESA, The 23rd ESLAB Symposium on Two Topics in X Ray Astronomy. Volume 1: X Ray Binaries p 633-640 (SEE N90-25711 19-89)

Astronomy and Astrophysics

Astronomy

1

Imaging Spectrometers, Magellanic Clouds, Mir Space Station, Supernova 1987A, X Ray Spectra, Radiant Flux Density, Spectrum Analysis, Stellar Spectra, Variability, X Ray Astronomy

Scientific paper

The results of the Large Magellanic Cloud (LMC) observations in the 2 to 30 keV band by the coded mask imaging spectrometer instrument of the Mir-Kvant X ray observatory are presented. The observations were performed during the period Nov. 1988 to Jun. 1989. An upper limit on the flux from supernova SN1987A is found to be 0.6 mCrab in this band. The results of monitoring and spectral observations of LMC X-1, LMC X-2, LMC X-3, LMC X-4 and PSR0540-693 are given.

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