Instabilities and Flow Structures in Protoplanetary Disks: Setting the Stage for Planetesimal Formation-Reference-Cited by-同舟云学术

Instabilities and Flow Structures in Protoplanetary Disks: Setting the Stage for Planetesimal Formation

Published:2018 Issue: Volume: Page:1-36
ISSN:
Container-title:Handbook of Exoplanets
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Author:

Klahr Hubert,Pfeil Thomas,Schreiber Andreas

Publisher

Springer International Publishing

Link

http://link.springer.com/content/pdf/10.1007/978-3-319-30648-3_138-1

Reference94 articles.

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2. Arlt R, Urpin V (2004) Simulations of vertical shear instability in accretion discs. Astron Astrophy 426(3):755–765. https://doi.org/10.1051/0004-6361:20035896

3. Armitage P (2013) Astrophysics of planet formation. Cambridge University Press. https://books.google.de/books?id=EFYOngEACAAJ

4. Avila M (2012) Stability and angular-momentum transport of fluid flows between corotating cylinders. Phys Rev Lett 108(12):124501

5. Bai XN, Stone JM (2013) Wind-driven accretion in protoplanetary disks. I. Suppression of the magnetorotational instability and launching of the magnetocentrifugal wind. ApJ 769(1):76

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