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Coma Southwest — as seen by the GMRT

Published online by Cambridge University Press:  26 May 2016

K. S. Dwarakanath  and
J.N. Chengalur
K. S. Dwarakanath
Affiliation:
Raman Research Institute, Bangalore 560080, India
J.N. Chengalur
Affiliation:
National Center for Radio Astrophysics, TIFR, Post Bag No 3, Ganeshkhind, Pune 41007, India

Abstract

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We have imaged in HI a ∼ 25′ field of view in the Coma Southwest region using the Giant Meterwave Radio Telescope. No HI was detected to a 3σ limit of 3 × 108M⊙ in the surveyed volume. Except for NGC 4839, no radio continuum emission was detected from the galaxies in the Coma Southwest to a 3σ limit of 3 × 1020 W Hz−1 of spectral luminosity at 1.4 GHz.

Type
Part 3: Clusters of Galaxies
Information
Symposium - International Astronomical Union , Volume 199: The Universe at Low Radio Frequencies , 2002 , pp. 166 - 167
Copyright
Copyright © Astronomical Society of the Pacific 2002 

References

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