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(Fe X) and (Fe XIV) emmision from Puppis A and other supernova remnants

Journal Article · · Astrophys. J.; (United States)
DOI:https://doi.org/10.1086/156902· OSTI ID:6251406
Measurements of (Fe XIV) 5303 A (Fe X) 6374 A emission from several supernova remnants are reported, and their relation to X-ray observations is discussed. The brightest (Fe XIV) emission region in Puppis A is interpreted as the result of the supernova shock wave interacting with a dense cloud in the interstellar medium.
Research Organization:
Goddard Space Flight Center, Greenbelt, Maryland
OSTI ID:
6251406
Journal Information:
Astrophys. J.; (United States), Journal Name: Astrophys. J.; (United States) Vol. 228:3; ISSN ASJOA
Country of Publication:
United States
Language:
English