X-ray observations of some radio supernova remnants by ANS

Details X-ray observations of some radio supernova remnants by ANS X-ray observations of some radio supernova remnants by ANS

Aug 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979a%26a....77...53g&link_type=abstract

Astronomy and Astrophysics, vol. 77, no. 1-2, Aug. 1979, p. 53-60.

Astronomy and Astrophysics

Astronomy

8

Interstellar Matter, Radio Sources (Astronomy), Satellite-Borne Instruments, Supernova Remnants, X Ray Spectra, Astronomical Catalogs, Astronomical Netherlands Satellite, Density Distribution, Energy Spectra, Stellar Luminosity

Scientific paper

With the X-ray instruments aboard the ANS satellite some radio supernova remnants (SNRs) have been observed in the energy ranges 0.16-0.284 keV and 0.32-7 keV. The observations resulted in upper limits for the luminosities from which it is possible to infer, on the basis of an adiabatic shock-wave model, the existence of a tenuous interstellar medium around some SNRs.

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