AGN Feedback in Galaxy Groups: A Joint GMRT/X-ray Study
被引:5
作者:
Giacintucci, S.
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Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USAHarvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA
Giacintucci, S.
[1
]
Vrtilek, J. M.
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Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USAHarvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA
Vrtilek, J. M.
[1
]
O'Sullivan, E.
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Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USAHarvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA
O'Sullivan, E.
[1
]
Raychaudhury, S.
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Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USAHarvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA
Raychaudhury, S.
[1
]
David, L. P.
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Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USAHarvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA
David, L. P.
[1
]
Venturi, T.
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Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USAHarvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA
Venturi, T.
[1
]
Athreya, R.
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Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USAHarvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA
Athreya, R.
[1
]
Gitti, M.
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Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USAHarvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA
Gitti, M.
[1
]
机构:
[1] Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA
来源:
MONSTER'S FIERY BREATH: FEEDBACK IN GALAXIES, GROUPS, AND CLUSTERS
|
2009年
/
1201卷
关键词:
Galaxy groups;
Radio galaxies;
X-ray observations;
CLUSTER AWM-4;
RADIO;
CORE;
D O I:
10.1063/1.3293043
中图分类号:
P1 [天文学];
学科分类号:
0704 ;
摘要:
We present an ongoing study of 18 nearby galaxy groups, chosen for the availability of Chandra and/or XMM-Newton data and evidence for AGN/hot intragroup gas interaction. We have obtained 235 and 610 MHz observations at the GMRT for all the groups, and 327 and 150 MHz for a few. We discuss two interesting cases - NGC 5044 and AWM4 - which exhibit different kinds of AGN/hot gas interaction. With the help of these examples we show how joining low-frequency radio data (to track the history of AGN outbursts through emission from aged electron populations) with X-ray data (to determine the state of hot gas, its disturbances, heating and cooling) can provide a unique insight into the nature of the feedback mechanism in galaxy groups.
机构:
Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA
Univ Roma Tor Vergata, Dipartimento Fis, I-00133 Rome, ItalyIst Radioastron, INAF, I-40129 Bologna, Italy
Mazzotta, Pasquale
;
Clarke, Tracy E.
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机构:
USN, Res Lab, Washington, DC 20375 USA
Interferometr Inc, Herndon, VA 20171 USAIst Radioastron, INAF, I-40129 Bologna, Italy
Clarke, Tracy E.
;
Athreya, Ramana M.
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机构:
Natl Ctr Radio Astrophys, Tata Inst Fundamental Res, Pune 411007, Maharashtra, IndiaIst Radioastron, INAF, I-40129 Bologna, Italy
机构:
Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA
Univ Roma Tor Vergata, Dipartimento Fis, I-00133 Rome, ItalyIst Radioastron, INAF, I-40129 Bologna, Italy
Mazzotta, Pasquale
;
Clarke, Tracy E.
论文数: 0引用数: 0
h-index: 0
机构:
USN, Res Lab, Washington, DC 20375 USA
Interferometr Inc, Herndon, VA 20171 USAIst Radioastron, INAF, I-40129 Bologna, Italy
Clarke, Tracy E.
;
Athreya, Ramana M.
论文数: 0引用数: 0
h-index: 0
机构:
Natl Ctr Radio Astrophys, Tata Inst Fundamental Res, Pune 411007, Maharashtra, IndiaIst Radioastron, INAF, I-40129 Bologna, Italy