We present an ongoing, low-frequency radio/X-ray study of 18 nearby galaxy groups, chosen for the evidence, either in the X-ray or radio images, of AGN/intragroup gas interaction. We have obtained radio observations at 235 MHz and 610 MHz with the Giant Metrewave Radio Telescope (GMRT) for all the groups, and 327 MHz and 150 MHz for a few. We present results of the recent Chandra/GMRT study of the interesting case of AWM 4, a relaxed poor cluster of galaxies with no evidence of a large cool core and no X-ray cavities associated with the central radio galaxy. Our analysis shows how joining low-frequency radio data (to track the history of AGN outbursts) with X-ray data (to determine the state of the hot gas, its disturbances, heating and coo...
Low frequency radio astronomy allows us to observe the fainter and older synchrotron emission from t...
The energy released by Active Galactic Nuclei (AGN) in the form of radiation, winds, or radio plasma...
Restricted Access. Articles older than 2 years are open to all at the journal site (alternative loca...
We present an ongoing, low-frequency radio/X-ray study of 18 nearby galaxy groups, chosen for the ev...
none15We present new Giant Metrewave Radio Telescope observations at 235 MHz and 610 MHz of 18 X-ray...
As a part of an ongoing study of a sample of galaxy groups showing evidence for AGN/hot gas interact...
Received — ; accepted — Abstract. Much of the evolution of galaxies takes place in groups where feed...
Our understanding of how active galactic nucleus feedback operates in galaxy clusters has improved i...
In the last two decades, significant improvements have been made in the understanding of how AGN fee...
We present new Giant Metrewave Radio Telescope observations at 235 MHz and 610 MHz of 18 X-ray brigh...
Galaxy clusters are the most massive bound objects in the universe. Roughly 90% of the baryons in cl...
Feedback by radio-loud active galactic nuclei (AGNs) in galaxy groups is not fully understood. Open ...
In this paper we analyze AGN activity signatures in the rich nearby galaxy cluster Abell 1795 aiming...
Low frequency radio astronomy allows us to observe the fainter and older synchrotron emission from t...
The energy released by Active Galactic Nuclei (AGN) in the form of radiation, winds, or radio plasma...
Restricted Access. Articles older than 2 years are open to all at the journal site (alternative loca...
We present an ongoing, low-frequency radio/X-ray study of 18 nearby galaxy groups, chosen for the ev...
none15We present new Giant Metrewave Radio Telescope observations at 235 MHz and 610 MHz of 18 X-ray...
As a part of an ongoing study of a sample of galaxy groups showing evidence for AGN/hot gas interact...
Received — ; accepted — Abstract. Much of the evolution of galaxies takes place in groups where feed...
Our understanding of how active galactic nucleus feedback operates in galaxy clusters has improved i...
In the last two decades, significant improvements have been made in the understanding of how AGN fee...
We present new Giant Metrewave Radio Telescope observations at 235 MHz and 610 MHz of 18 X-ray brigh...
Galaxy clusters are the most massive bound objects in the universe. Roughly 90% of the baryons in cl...
Feedback by radio-loud active galactic nuclei (AGNs) in galaxy groups is not fully understood. Open ...
In this paper we analyze AGN activity signatures in the rich nearby galaxy cluster Abell 1795 aiming...
Low frequency radio astronomy allows us to observe the fainter and older synchrotron emission from t...
The energy released by Active Galactic Nuclei (AGN) in the form of radiation, winds, or radio plasma...
Restricted Access. Articles older than 2 years are open to all at the journal site (alternative loca...