AGN Feedback in galaxy groups: a detailed study of X-ray features and diffuse radio emission in IC1262

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Main Authors: Pandge, M. B., Sonkamble, S. S., Parekh, Viral, Dabhade, Pratik, Parmar, Avni, Patil, M. K., Raychaudhury, Somak
Format: Preprint
Published: 2018
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author Pandge, M. B.
Sonkamble, S. S.
Parekh, Viral
Dabhade, Pratik
Parmar, Avni
Patil, M. K.
Raychaudhury, Somak
author_facet Pandge, M. B.
Sonkamble, S. S.
Parekh, Viral
Dabhade, Pratik
Parmar, Avni
Patil, M. K.
Raychaudhury, Somak
contents This paper reports a systematic search of X-ray cavities, density jumps and shocks in the inter-galactic environment of the galaxy group IC~1262 using {\it Chandra}, GMRT and VLA archival observations. The X-ray imaging analysis reveals a pair of X-ray cavities on the north and south of the X-ray peak, at projected distances of 6.48\,kpc and 6.30\,kpc respectively. Total mechanical power contained in both these cavities is found to be $\sim$12.37$\times 10^{42}$ erg~s$^{-1}$, and compares well with the X-ray luminosity, within the cooling radius, measured to be $\sim 3.29 \times 10^{42}$ erg~s$^{-1}$, suggesting that the mechanical power injected by the central AGN efficiently balances the radiative loss. We detect a previously unknown X-ray cavity at the position of southern radio lobe in the intra-group medium and find a loop of excess X-ray emission extending $\sim$100 kpc southwest from the central galaxy. The X-ray cavity at the position of southern radio lobe probably represents a first generation X-ray cavity. Two surface brightness edges are evident to the west and east$-$north of the center of this group. The radio galaxy at the core of the IC~1262 group is a rare low-redshift ultra-steep radio galaxy, its spectral index being $α\! \sim\! -1.73$ (including the central AGN) and $α\! \sim\! -2.08$ (excluding the central AGN). We detect a radio phoenix embedded within the southern radio lobe, for the first time in a poor group, with a spectral index ($α\!\leq\! -1.92$). The spectral index distribution across the phoenix steepens with increasing distance from its intensity peak.
format Preprint
id arxiv_https___arxiv_org_abs_1811_05647
institution arXiv
publishDate 2018
record_format arxiv
spellingShingle AGN Feedback in galaxy groups: a detailed study of X-ray features and diffuse radio emission in IC1262
Pandge, M. B.
Sonkamble, S. S.
Parekh, Viral
Dabhade, Pratik
Parmar, Avni
Patil, M. K.
Raychaudhury, Somak
Astrophysics of Galaxies
Cosmology and Nongalactic Astrophysics
This paper reports a systematic search of X-ray cavities, density jumps and shocks in the inter-galactic environment of the galaxy group IC~1262 using {\it Chandra}, GMRT and VLA archival observations. The X-ray imaging analysis reveals a pair of X-ray cavities on the north and south of the X-ray peak, at projected distances of 6.48\,kpc and 6.30\,kpc respectively. Total mechanical power contained in both these cavities is found to be $\sim$12.37$\times 10^{42}$ erg~s$^{-1}$, and compares well with the X-ray luminosity, within the cooling radius, measured to be $\sim 3.29 \times 10^{42}$ erg~s$^{-1}$, suggesting that the mechanical power injected by the central AGN efficiently balances the radiative loss. We detect a previously unknown X-ray cavity at the position of southern radio lobe in the intra-group medium and find a loop of excess X-ray emission extending $\sim$100 kpc southwest from the central galaxy. The X-ray cavity at the position of southern radio lobe probably represents a first generation X-ray cavity. Two surface brightness edges are evident to the west and east$-$north of the center of this group. The radio galaxy at the core of the IC~1262 group is a rare low-redshift ultra-steep radio galaxy, its spectral index being $α\! \sim\! -1.73$ (including the central AGN) and $α\! \sim\! -2.08$ (excluding the central AGN). We detect a radio phoenix embedded within the southern radio lobe, for the first time in a poor group, with a spectral index ($α\!\leq\! -1.92$). The spectral index distribution across the phoenix steepens with increasing distance from its intensity peak.
title AGN Feedback in galaxy groups: a detailed study of X-ray features and diffuse radio emission in IC1262
topic Astrophysics of Galaxies
Cosmology and Nongalactic Astrophysics
url https://arxiv.org/abs/1811.05647