Coronal lines in supernova remnant spectra

Details Coronal lines in supernova remnant spectra Coronal lines in supernova remnant spectra

Jun 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978mnras.183p..79m&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 183, June 1978, p. 79P-84P.

Astronomy and Astrophysics

Astronomy

5

Coronas, Forbidden Bands, Line Spectra, Supernova Remnants, Interstellar Magnetic Fields, Plasma Heating, Shock Heating, Shock Waves, Signal To Noise Ratios, Synchrotron Radiation, Thermal Radiation, X Ray Astronomy

Scientific paper

The detection of coronal line emission offers the possibility of studying the shock-heated plasma in supernova remnants (SNRs). A search was performed for the 5303-A forbidden Fe XIV coronal line in the SNRs N49 and Vela. The line was detected in the former at an intensity suggesting a plasma temperature in the region of 2 million K. However, a previously proposed detection for the Vela SNR was not confirmed.

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