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Observations of Straight-angle Tailed Radio Galaxies in Rich Clusters of Galaxies

Published online by Cambridge University Press:  25 May 2016

Aileen A. O'Donoghue ,
Jean A. Eilek  and
Frazer N. Owen
Aileen A. O'Donoghue
Affiliation:
St. Lawrence University, Canton, New York 13617 USA New Mexico Institute of Mining and Technology Socorro, New Mexico 87801 USA NRAO-VLA, Socorro, New Mexico 87801 USA
Jean A. Eilek
Affiliation:
St. Lawrence University, Canton, New York 13617 USA New Mexico Institute of Mining and Technology Socorro, New Mexico 87801 USA NRAO-VLA, Socorro, New Mexico 87801 USA
Frazer N. Owen
Affiliation:
St. Lawrence University, Canton, New York 13617 USA New Mexico Institute of Mining and Technology Socorro, New Mexico 87801 USA NRAO-VLA, Socorro, New Mexico 87801 USA

Extract

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We have begun VLA observations of straight-angle tailed radio sources (SATs) at 1.5 and 4.8 GHz (L and C band) to achieve one arcsecond resolution at each frequency. This will provide a SAT data set similar to the O'Donoghue, Owen, and Eilek (1990) WAT data set with both total intensity and spectral index information. We will use these data to examine morphological and dynamical properties of straight-tailed radio sources in clusters of galaxies.

Type
Radio Sources and their Environment
Information
Symposium - International Astronomical Union , Volume 175: Extragalactic Radio Sources , 1996 , pp. 349 - 350
Copyright
Copyright © Kluwer 1996 

References

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