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X-ray emission from the supernova remnant MSH 14-63X-ray emission in the 0.6-2.5-keV energy range has been detected from the supernova remnant MSH 14-63. The observed flux is 3.5 by 10 to the -10th power erg/sq cm per sec. The absence of lower-energy X-rays indicates a hydrogen column density consistent with the radio and optical distance estimates of 2.5 kpc.
Document ID
19770047185
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
doi:10.1086/182408
Authors
Naranan, S. (Hulburt (E. O.) Center for Space Research Washington, DC, United States)
Shulman, S. (Hulburt (E. O.) Center for Space Research Washington, DC, United States)
Yentis, D. (Hulburt (E. O.) Center for Space Research Washington, DC, United States)
Fritz, G. (Hulburt (E. O.) Center for Space Research Washington, DC, United States)
Friedman, H. (U.S. Navy, E. O. Hulburt Center for Space Research, Washington D.C., United States)
Date Acquired
August 8, 2013
Publication Date
April 15, 1977
Publication Information
Publication: Astrophysical Journal
Subject Category
Astronomy
Accession Number
77A30037
Funding Number(s)
CONTRACT_GRANT: NASA ORDER T-845-C
Distribution Limits
Public
Copyright
Other

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