The influence of winds on the time-dependent behaviour of self-gravitating accretion discs
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/395/2/877/4886522/mnras0395-0877.pdf
Reference28 articles.
1. Outflows and Jets from Collapsing Magnetized Cloud Cores
2. Massive Star Formation via High Accretion Rates and Early Disk‐driven Outflows
3. Advection‐dominated Accretion with Infall and Outflows
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1. The influence of realistic cooling on the structure and spectrum of self-gravitating protoplanetary discs;The European Physical Journal Plus;2024-05-28
2. The self-similar structure of advection-dominated discs with outflow and radial viscosity;Monthly Notices of the Royal Astronomical Society;2020-03-03
3. Self-gravity in magnetized accretion discs as a result of a dynamo mechanism with outflows;Monthly Notices of the Royal Astronomical Society;2020-02-29
4. Time-dependent Study of a Protoplanetary Disk with a Magnetic Prandtl Number;The Astrophysical Journal;2018-08-10
5. VISCOUS ACCRETION OF A POLYTROPIC SELF-GRAVITATING DISK IN THE PRESENCE OF WIND;The Astrophysical Journal;2013-02-21
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