Published April 15, 1974 | Version v1
Journal article

The correlation of radio emission and optical type with x-ray emission from clusters of galaxies

Creators

  • 1. University of Texas Radio Astronomy Observatory, Department of Astronomy, University of Texas at Austin, Austin, Texas

Description

view Abstract Citations (36) References (24) Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS The Correlation of Radio Emission and Optical Type with X-Ray Emission from Clusters of Galaxies Owen, Frazer N. Abstract A correlation of X-ray emission from clusters of galaxies with radio emission and with Rood and Sastry optical cluster type is reported. Of the 10 clusters with the highest known absolute X-ray luminosity, at least nine are strong radio sources. Also, eight of these 10 clusters are characterized by Rood and Sastry as containing one or two outstanding dominant galaxies. In light of these correlations the two most likely X-ray emission mechanisms-inverse Compton scattering and thermal bremsstrahlung-are discussed. Subject headings: galaxies, clusters of - radio sources - X-ray sources Publication: The Astrophysical Journal Pub Date: April 1974 DOI: 10.1086/181463 Bibcode: 1974ApJ...189L..55O full text sources ADS | data products SIMBAD (10)

Additional details

Additional titles

Augmented title (English)
Larger sample, thermal bremsstrahlung

Identifiers

Publishing Information

Journal Title
The Astrophysical Journal
Journal Volume
189
Journal Issue
2
Series
Astrophys. J., Lett.
Journal Page Range
L55
ISSN
0004-637X

Optional Information

Notes
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