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The megaparsec radio relic in supercluster, Rood No. 27Observations of extended source of low surface brightness appear as a 'relic' of a currently inactive radio galaxy. The largest dimension is approximately 1.6 Mpc, the fractional polarization is high, and the magnetic field direction appears to be coherent over scales of at least several hundred kpc. Polarization and morphologies of relics are distinct from those of cluster halos, due to the different environment provided by cluster cores compared to that encountered in the outer fringes of the hot gas distribution which produces X-ray emission.
Document ID
19930046154
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Harris, D. E.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Stern, C. P.
(Harvard-Smithsonian Center for Astrophysics Cambridge, MA, United States)
Willis, A. G.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Dewdney, P. E.
(Dominion Radio Astrophysical Observatory Penticton, Canada)
Date Acquired
August 16, 2013
Publication Date
March 1, 1993
Publication Information
Publication: Astronomical Journal
Volume: 105
Issue: 3
ISSN: 0004-6256
Subject Category
Astrophysics
Accession Number
93A30151
Funding Number(s)
CONTRACT_GRANT: NAS8-30751
Distribution Limits
Public
Copyright
Other

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