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High-resolution radio observations of the supernova remnant G24.7 + 0.6 and the discovery of an ultracompact H II regionThe Crab-like SNR G24.7 + 0.6 with 12 arcmin resolution at 20 cm wavelength has been observed. The image reveals a bright Crab-like core surrounded by a faint shell. An ultracompact H II region lies adjacent to the remnant core and several other compact H II regions lie just outside the remnant shell. Optical, far-infrared, and X-ray observations of the region are also presented. The specific attributes of this remnant and its place in the classification of composite versus Crab-like remnants as well as the general question of the association between Crab-like remnants and H II regions are discussed.
Document ID
19870053391
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Becker, R. H.
(California, University Davis and Livermore, United States)
Helfand, D. J.
(Columbia University New York, United States)
Date Acquired
August 13, 2013
Publication Date
May 15, 1987
Publication Information
Publication: Astrophysical Journal, Part 1
Volume: 316
ISSN: 0004-637X
Subject Category
Astrophysics
Accession Number
87A40665
Funding Number(s)
CONTRACT_GRANT: JPL-957252
CONTRACT_GRANT: AF-AFOSR-82-0014
CONTRACT_GRANT: NSF AST-84-19370
CONTRACT_GRANT: NAG8-579
CONTRACT_GRANT: NAG8-558
Distribution Limits
Public
Copyright
Other

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