Radiatively Inefficient Accretion Flows with Outflow

Chin. Phys. Lett.

2006, Vol. 23

Issue (2): 523-526 DOI:

Original Articles

Radiatively Inefficient Accretion Flows with Outflow

XUE Li^1,2,3;WANG Jian-Cheng^1,2;LU Ju-Fu⁴

¹National Astronomical Observatories/Yunnan Astronomical Observatory, Chinese Academy of Sciences, Kunming 650011 ²United Laboratory of Optical Astronomy, Chinese Academy of Sciences, Kunming 650011 ³Graduate School of Chinese Academy of Sciences, Beijing 100039 ⁴Department of Physics, Xiamen University, Xiamen 361005

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XUE Li, WANG Jian-Cheng, LU Ju-Fu 2006 Chin. Phys. Lett. 23 523-526

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Abstract We construct a family of self-similar solutions to describe radiatively inefficient accretion flows with outflow. We show that outflow has important effects on the dynamical structure of accretion flows. In particular, we prove that outflow can be an effective mechanism of removing the released gravitational energy of accreted gas.

Keywords: 97.60.Lf 98.62.Mw 95.30.Gv

Published: 01 February 2006

PACS:	97.60.Lf	(Black holes)
	98.62.Mw	(Infall, accretion, and accretion disks)
	95.30.Gv	(Radiation mechanisms; polarization)

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https://cpl.iphy.ac.cn/ OR https://cpl.iphy.ac.cn/Y2006/V23/I2/0523

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