Tailed Radio Galaxies as Environmental Probes

Details Tailed Radio Galaxies as Environmental Probes Tailed Radio Galaxies as Environmental Probes

Sep 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011soust..50c..10d&link_type=abstract

Southern Stars. The Journal of the Royal Astronomical Society of New Zealand (ISSN 0049-1640), Vol. 50, No. 3, p. 10 - 12, (2011

Astronomy and Astrophysics

Astronomy

Galaxies: Active, Radio Continuum: Galaxies, Galaxies: General, Galaxies: Clusters: General

Scientific paper

We provide a brief overview of tailed radio galaxies and discuss how their morphology relates to the environment in which they reside. We report on the initial results of our simulations on the galaxy PKS J0334-3900 which show that a combination of cluster weather and orbital motion are required to generate the observed radio tails. Finally we show 12 newly detected HT galaxies in the Chandra Deep Field-South, including galaxy S447 - the most distant HT ever found.

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