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ATLAS, and wide-angle tail galaxies in ATLAS

Citation

Mao, MY and Sharp, R and Saikia, DJ and Norris, RP and Johnston-Hollitt, M and Middelberg, E and Lovell, JEJ, ATLAS, and wide-angle tail galaxies in ATLAS, Journal of Astrophysics and Astronomy, 32, (4) pp. 585-588. ISSN 0250-6335 (2011) [Refereed Article]


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Copyright Statement

Copyright 2011 Indian Academy of Sciences

DOI: doi:10.1007/s12036-011-9115-3

Abstract

Using the Australia Telescope Compact Array (ATCA), ATLAS (Australia Telescope Large Area Survey) is imaging two fields totalling 7 square degrees down to 10 μJy beam − 1 at 1.4 GHz. We have found 6 wide-angle tail galaxies (WATs), 4 of which have sufficient data to identify associated galaxy overdensities. The largest WAT, at a red-shift of 0.22, appears to be associated with an overdensity of galaxies that is spread over an unusually large extent of 12 Mpc, with a velocity range of 4500 km s − 1. Here we present the WATs in ATLAS and discuss the implications of these observations for future large-scale radio surveys such as ASKAP-EMU.

Item Details

Item Type:Refereed Article
Keywords:galaxies: clusters: general, galaxies: active, galaxies: general, radio continuum: galaxies, galaxies: distances and red-shifts
Research Division:Physical Sciences
Research Group:Astronomical and Space Sciences
Research Field:Cosmology and Extragalactic Astronomy
Objective Division:Expanding Knowledge
Objective Group:Expanding Knowledge
Objective Field:Expanding Knowledge in the Physical Sciences
Author:Mao, MY (Miss Minnie Mao)
Author:Lovell, JEJ (Dr Jim Lovell)
ID Code:98505
Year Published:2011
Web of Science® Times Cited:5
Deposited By:Mathematics and Physics
Deposited On:2015-02-18
Last Modified:2017-11-03
Downloads:213 View Download Statistics

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