Soft X-ray sources in the bar of the Large Magellanic Cloud

Details Soft X-ray sources in the bar of the Large Magellanic Cloud Soft X-ray sources in the bar of the Large Magellanic Cloud

May 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980apj...238...93m&link_type=abstract

Astrophysical Journal, Part 1, vol. 238, May 15, 1980, p. 93-97.

Astronomy and Astrophysics

Astrophysics

4

Astrophysics, Magellanic Clouds, X Ray Sources, Angular Resolution, Luminosity, Rocket-Borne Instruments, Supernova Remnants

Scientific paper

X-ray observations of the Large Magellanic Cloud were made with two collimated proportional counters having high angular resolution, a wide spectral dynamic range and a large aperture. Counting rates in the two detectors during the entire rocket flight are presented, and a number of soft X-ray (0.5-2 keV) sources were found in the bar of the LMC, having luminosities between 10 to the 37th and 10 to the 38th ergs/s. Emission in the 0.15-0.28 keV band from LMC X-3 was also detected.

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