A radio minihalo in the extreme cool-core galaxy cluster RXC J1504.1-0248
Abstract
Aims: We report the discovery of a radio minihalo in RXC J1504.1-0248, a massive galaxy cluster that has an extremely luminous cool core. To date, only 9 radio minihalos are known, thus the discovery of a new one in one of the most luminous cool-core clusters provides important information on this peculiar class of sources and sheds light on their origin.
Methods: The diffuse radio source was detected using GMRT at 327 MHz and confirmed by pointed VLA data at 1.46 GHz. The minihalo has a radius of ~140 kpc. A Chandra gas temperature map shows that the minihalo emission fills the cluster cool core and has some morphological similarities to it, as has been previously observed for other minihalos.
Results: The Chandra data reveal two subtle cold fronts in the cool core, likely created by sloshing of the core gas, as observed in most cool-core clusters. Following previous work, we speculate that the origin of the minihalo is related to sloshing. Sloshing may result in particle acceleration by generating turbulence and/or amplifying the magnetic field in the cool core, leading to the formation of a minihalo.
- Publication:
-
Astronomy and Astrophysics
- Pub Date:
- January 2011
- DOI:
- 10.1051/0004-6361/201015882
- arXiv:
- arXiv:1011.3141
- Bibcode:
- 2011A&A...525L..10G
- Keywords:
-
- radiation mechanisms: non-thermal;
- galaxies: clusters: general;
- galaxies: clusters: individual: RXC J1504.1-0248;
- Astrophysics - High Energy Astrophysical Phenomena;
- Astrophysics - Cosmology and Nongalactic Astrophysics
- E-Print:
- 4 pages, 1 table, 3 color figures. Accepted for publication in A&