pith. sign in

arxiv: 1203.0538 · v1 · pith:YEHRDALDnew · submitted 2012-03-02 · 🌌 astro-ph.GA

CGCG 292-057 - a radio galaxy with merger-modulated radio activity

classification 🌌 astro-ph.GA
keywords radiogalaxyactivitycgcgfeatureshighlysourcealmost
0
0 comments X p. Extension
pith:YEHRDALD Add to your LaTeX paper What is a Pith Number?
\usepackage{pith}
\pithnumber{YEHRDALD}

Prints a linked pith:YEHRDALD badge after your title and writes the identifier into PDF metadata. Compiles on arXiv with no extra files. Learn more

read the original abstract

We announce the discovery of a unique combination of features in a radio source identified with the merger galaxy CGCG 292-057. The radio galaxy both exhibits a highly complex, X-like structure and shows signs of recurrent activity in the form of double-double morphology. The outer lobes of CGCG 292-057 are characterized by low radio power, P_{1400MHz} \simeq 2 * 10^{24} W\Hz^{-1}, placing this source below the FRII/FRI luminosity threshold, and are highly polarized (almost 20 per cent at 1400 MHz) as is typical of X-shaped radio sources. The host is a LINER-type galaxy with a relatively low black hole mass and double-peaked narrow emission lines. These features make this galaxy a primary target for studies of merger-triggered radio activity.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.