Characterizing gravito-turbulence in 3D: turbulent properties and stability against fragmentation-Reference-Cited by-同舟云学术

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Characterizing gravito-turbulence in 3D: turbulent properties and stability against fragmentation

Published:2018-12-10 Issue:3 Volume:483 Page:3718-3729
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Booth Richard A¹^ORCID,Clarke Cathie J¹

Affiliation:

1. Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA, UK

Funder

European Research Council

BIS National E-infrastructure capital

Science and Technology Facilities Council

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/483/3/3718/27299904/sty3340.pdf

Reference63 articles.

1. The Fragmentation Criteria in Local Vertically Stratified Self-gravitating Disk Simulations

2. A TWO-COMPONENT POWER LAW COVERING NEARLY FOUR ORDERS OF MAGNITUDE IN THE POWER SPECTRUM OF SPITZER FAR-INFRARED EMISSION FROM THE LARGE MAGELLANIC CLOUD

3. The Thermal Regulation of Gravitational Instabilities in Protoplanetary Disks. III. Simulations with Radiative Cooling and Realistic Opacities

4. Collision velocity of dust grains in self-gravitating protoplanetary discs

5. Evolution of the Solar Nebula. IV. Giant Gaseous Protoplanet Formation

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