Evidence of X-ray emission from W44

Details Evidence of X-ray emission from W44 Evidence of X-ray emission from W44

Apr 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978a%26a....65l...9g&link_type=abstract

Astronomy and Astrophysics, vol. 65, no. 2, Apr. 1978, p. L9-L12.

Astronomy and Astrophysics

Astronomy

6

Luminous Intensity, Satellite Observation, Supernova Remnants, X Ray Sources, Astronomical Models, Astronomical Netherlands Satellite, Radio Sources (Astronomy), Signal To Noise Ratios, Spaceborne Astronomy, X Ray Astronomy

Scientific paper

The Astronomical Netherlands Satellite (ANS) has provided X-ray observations around the supernova remnant W44. X-ray emission with an observed intensity of 8 x 10 to the -11th power erg/sq cm/s (i.e., 1.03-3.5 keV) has been detected from a region which overlaps the radio source. Spectral fits to the pulse-height data and the application of the shock-wave model for the evolution of the signal-to-noise ratio suggest that W44 is the X-ray source.

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