Publication Date:
2011-08-17
Description:
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.
Keywords:
ASTRONOMY
Type:
Astrophysical Journal; vol. 228
Format:
text
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