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

Wind production from thin accretion disk

1 Mar 2021, 11:00
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

Speakers

Ms Weixiao WangDr Defu Bu

Description

Strong winds are common phenomena in active galactic nuclei. Although, there are abundant observational data about winds, the launching mechanisms of the winds are still not clear. Two possible drving mechanisms are radiation line force driven and magnetic driven. I will talk about our recent numerical simulation work on the roles of the two mechanisms on driving winds.

Primary authors

Presentation materials

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