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Outflows from black hole accretion flows with various accretion rates

Published online by Cambridge University Press:  28 October 2024

De-Fu Bu Open the ORCID record for De-Fu Bu [Opens in a new window]  and
Feng Yuan
De-Fu Bu*
Affiliation:
Shanghai Astronomical Observatory, Chinese Academy of Sciences, 80 Nandan Road, Shanghai 200030, China
Feng Yuan*
Affiliation:
Shanghai Astronomical Observatory, Chinese Academy of Sciences, 80 Nandan Road, Shanghai 200030, China
*
email: dfbu@shao.ac.cn, fyuan@shao.ac.cn
email: dfbu@shao.ac.cn, fyuan@shao.ac.cn
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Abstract

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Both observations and theoretical studies have convincingly shown that outflows (i.e., wind and jet) are common phenomena from black hole accretion systems with various accretion rates, although the physical driving mechanisms are not exactly same for different accretion modes. Outflows are not only important in the dynamics of black hole accretion, but also play an important role in AGN feedback; therefore it is crucial to investigate their main physical properties including mass flux and velocity. In this paper we summarize recent studies in investigating the properties and driving mechanisms from black hole accretion flows with various accretion rates.

Keywords

accretionaccretion discsblack hole physicshydrodynamics
Type
Contributed Paper
Information
Proceedings of the International Astronomical Union , Volume 19 , Symposium S378: Black Hole Winds at All Scales , December 2023 , pp. 104 - 107
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Copyright
© The Author(s), 2024. Published by Cambridge University Press on behalf of International Astronomical Union

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