In-Depth Chandra Study of the AGN Feedback in Virgo Elliptical Galaxy M84

In-Depth Chandra Study of the AGN Feedback in Virgo Elliptical Galaxy M84
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钱德拉对处女座椭圆星系 M84 中 AGN 反馈的深入研究

DOI:
10.1086/591662
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发表时间:
2008
期刊:
The Astrophysical Journal
影响因子:
--
通讯作者:
Mandel
Mandel
中科院分区:
--
文献类型:
--
作者:
Finoguenov;Ruszkowski;Br¨ uggen;Vikhlinin;Mandel

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Using deep Chandra observations of M84, we study the energetics of the interaction between the black hole and the interstellar medium of this early-type galaxy. We perform a detailed two-dimensional reconstruction of the properties of the X-ray-emitting gas using a constrained Voronoi tessellation method, identifying the mean trends and carrying out the fluctuation analysis of the thermodynamical properties of the hot ISM. In addition to the PV work associated with the bubble expansion, we identify and measure the wave energy associated with the mildly supersonic bubble expansion. We show that, depending on the age of the cavity and the associated wave, the waves can make a substantial contribution to the total energy release from the AGN. The energy dissipated in the waves tends to be concentrated near the center of M84 and in the direction perpendicular to the bubble outflow, possibly due to the interference of the waves generated by the expansion of northern and southern bubbles. We also find direct evidence for the escape of radio plasma from the ISM of the host galaxy into the intergalactic medium.
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