NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Back to Results
The prevalence of supernova remnants among unidentified Galactic radio sourcesNine Galactic radio sources were mapped to identify new Crab-like and composite supernova remnants. The sources were selected on the basis of existing stringent upper limits on their hydrogen recombination line fluxes. One new Cracb-like remnant, one new composite remnant, at least one, and probably two, new shell-like remnants, and a compact H II region were found, along with the expected collection of extragalactic objects. The results suggest that there are several hundred SNRs in the Galaxy which are detectable with current instruments, but which have yet to be identified.
Document ID
19890053992
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Helfand, David J.
(Columbia University New York, United States)
Velusamy, T.
(Tata Institute for Fundamental Research Bombay, India)
Becker, R. H.
(California, University Davis; Lawrence Livermore National Laboratory, Livermore, CA, United States)
Lockman, Felix J.
(National Radio Astronomy Observatory Charlottesville, VA, United States)
Date Acquired
August 14, 2013
Publication Date
June 1, 1989
Publication Information
Publication: Astrophysical Journal, Part 1
Volume: 341
ISSN: 0004-637X
Subject Category
Astrophysics
Accession Number
89A41363
Funding Number(s)
CONTRACT_GRANT: NAG8-664
CONTRACT_GRANT: NSF AST-86-17184
CONTRACT_GRANT: JPL-95762
Distribution Limits
Public
Copyright
Other

Available Downloads

There are no available downloads for this record.
No Preview Available