X-ray emission from the supernova remnant MSH 14-63

Details X-ray emission from the supernova remnant MSH 14-63 X-ray emission from the supernova remnant MSH 14-63

Apr 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977apj...213l..53n&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor, vol. 213, Apr. 15, 1977, p. L53-L56.

Astronomy and Astrophysics

Astronomy

15

Energy Spectra, Radio Sources (Astronomy), Spaceborne Astronomy, Supernova Remnants, X Ray Sources, Continuous Radiation, Fine Structure, Histograms, Hydrogen Clouds, Nebulae, Pulsars, Radiant Flux Density

Scientific paper

X-ray emission in the 0.6-2.5-keV energy range has been detected from
the supernova remnant MSH 14-63. The observed flux is 3.5 by 10 to the
-10th power erg/sq cm per sec. The absence of lower-energy X-rays
indicates a hydrogen column density consistent with the radio and
optical distance estimates of 2.5 kpc.

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