Forbidden Fe X and forbidden Fe XIV emission from Puppis A and other supernova remnants

Details Forbidden Fe X and forbidden Fe XIV emission from Puppis A and other supernova remnants Forbidden Fe X and forbidden Fe XIV emission from Puppis A and other supernova remnants

Mar 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979apj...228..763l&link_type=abstract

Astrophysical Journal, Part 1, vol. 228, Mar. 15, 1979, p. 763-770. NASA-supported research.

Astronomy and Astrophysics

Astrophysics

31

Forbidden Bands, Iron, Nebulae, Shock Wave Interaction, Supernova Remnants, X Ray Sources, Astronomical Spectroscopy, Emission Spectra, Fine Structure, Interstellar Matter, Plasma Clouds

Scientific paper

Measurements of Fe XIV 5303-A and Fe X 6374-A forbidden emission from
several supernova remnants are reported, and their relation to X-ray
observations is discussed. The brightest Fe XIV forbidden-emission
region in Puppis A is interpreted as being the result of the supernova
shock wave's interacting with a dense cloud in the interstellar medium.

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