Radiation Hydrodynamical Turbulence in Protoplanetary Disks: Numerical Models and Observational Constraints-Reference-Cited by-同舟云学术

Radiation Hydrodynamical Turbulence in Protoplanetary Disks: Numerical Models and Observational Constraints

Published:2017-11-27 Issue:2 Volume:850 Page:131
ISSN:1538-4357
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Flock Mario^ORCID,Nelson Richard P.,Turner Neal J.^ORCID,Bertrang Gesa H.-M.,Carrasco-González Carlos,Henning Thomas,Lyra Wladimir^ORCID,Teague Richard^ORCID

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/850/i=2/a=131/pdf

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2. RINGED SUBSTRUCTURE AND A GAP AT 1 au IN THE NEAREST PROTOPLANETARY DISK

3. Simulations of vertical shear instability in accretion discs

4. SELF-DESTRUCTING SPIRAL WAVES: GLOBAL SIMULATIONS OF A SPIRAL-WAVE INSTABILITY IN ACCRETION DISKS

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