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1–3 Mar 2021
Tsung-Dao Lee Institute (East wing of Pao Yue-Kong Library)
Asia/Shanghai timezone

Wind and jet from black hole hot accretion flows

1 Mar 2021, 10:30
30m
East wing of Pao Yue-Kong Library/2nd-200 - 200# Meeting Room (Tsung-Dao Lee Institute (East wing of Pao Yue-Kong Library))

East wing of Pao Yue-Kong Library/2nd-200 - 200# Meeting Room

Tsung-Dao Lee Institute (East wing of Pao Yue-Kong Library)

800 Dongchuan Road, Minhang District
60

Speaker

Hai Yang (SHAO)

Description

Hot accretion flows around black holes can produce strong wind. These winds are important not only because they are an important ingredient in accretion dynamics, but also play an important role in AGN feedback. In this talk, we will first briefly review the history of wind study, then focus on introducing the properties of wind such as its mass flux and velocity. These properties are obtained by analyzing the 3D GRMHD numerical simulation data using a virtual particle trajectory approach. At last, we will compare the properties of wind and jet.

Primary author

Hai Yang (SHAO)

Co-author

Feng Yuan (Shanghai Astronomical Observatory)

Presentation materials

There are no materials yet.