Radio emission from the 2006 - 56 region
Open Access
- 1 January 1982
- journal article
- research article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 198 (1) , 259-264
- https://doi.org/10.1093/mnras/198.1.259
Abstract
The steep-spectrum radio source 2006–56 has been mapped with the Fleurs Synthesis Telescope at 1415 MHz with a resolution of 50 arcsec. The radio source is associated with a rich irregular cluster and consists of two possible head–tail objects and diffuse emission with a size of ∼ 2 Mpc (H = 50 km s−1 Mpc−1). Detection of the new head–tail sources adds to the unbiased sample of tailed sources needed to examine the importance of galaxy environment.Keywords
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