MRI and Outflows: Angular Momentum Transport in Protoplanetary Disks

Paper


Salmeron, Raquel. 2009. "MRI and Outflows: Angular Momentum Transport in Protoplanetary Disks ." Astrophysics and Space Science. Springer. https://doi.org/10.1007/978-3-642-00576-3_92
Paper/Presentation Title

MRI and Outflows: Angular Momentum Transport in Protoplanetary Disks

Presentation TypePaper
AuthorsSalmeron, Raquel
Journal or Proceedings TitleProtostellar Jets in Context
ERA Conference ID76741
Journal Citationpp. 611-613
Number of Pages3
Year2009
PublisherSpringer
ISBN9783642005763
9783642005756
9783642261176
Digital Object Identifier (DOI)https://doi.org/10.1007/978-3-642-00576-3_92
Web Address (URL) of Paperhttps://link.springer.com/chapter/10.1007/978-3-642-00576-3_92
Web Address (URL) of Conference Proceedingshttps://link.springer.com/book/10.1007/978-3-642-00576-3?page=6#toc
Conference/EventAstrophysics and Space Science
Event Details
Astrophysics and Space Science
Abstract

Angular momentum in protostellar disks can be transported radially by MHD turbulence induced by the magnetorotational instability (MRI); or vertically, via magnetocentrifugal outflows. We have studied these processes under realistic fluid conditions and explored the possibility that they operate at the same radial location. The results suggest that they may be unlikely to coexist in real disks.

KeywordsRadial Location; Protoplanetary Disk; Planet Formation; Sonic Point; Radial Transport
ANZSRC Field of Research 2020510107. Planetary science (excl. solar system and planetary geology)
SeriesAstrophysics and Space Science Proceedings (ASSSP)
Byline AffiliationsAustralian National University
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