Einstein X-ray observations of the Monoceros supernova remnant

Details Einstein X-ray observations of the Monoceros supernova remnant Einstein X-ray observations of the Monoceros supernova remnant

Mar 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985mnras.213p..15l&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 213, March 1, 1985, p. 15P-19P. Sponsorship: National S

Astronomy and Astrophysics

Astronomy

5

Brightness Distribution, Heao 2, Supernova Remnants, X Ray Imagery, X Ray Sources, Astronomical Maps, Proportional Counters

Scientific paper

The Monoceros nebula is seen in the optical and radio wavelengths as a ring of 3.5° angular diameter and is believed to be an old supernova remnant (SNR). The authors report the first positive detection of X-rays from the Monoceros nebula, confirming its supernova remnant nature. Reprocessed Einstein imaging proportional counter observations of soft X-rays (0.2 - 5 keV) were used to produce a contour map of the surface brightness distribution.

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