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Cited article:

The formation of a gas giant planet in a viscously evolved protoplanetary disk within the core accretion model

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Astrophysics and Space Science 363 (9) (2018)
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The evolution of the protoplanetary disk with mass influx from a molecular cloud core and the photoevaporation winds

Chunjian Liu, Zhen Yao, Hongna Li and Haosen Wang
New Astronomy 58 72 (2018)
https://doi.org/10.1016/j.newast.2017.07.009

The ability of a protostellar disc to fragment and the properties of molecular cloud cores

Chunjian Liu, Min Li, Zhen Yao and Xiaodong Mao
Astrophysics and Space Science 362 (1) (2017)
https://doi.org/10.1007/s10509-016-2986-7

Masses of discs form from collapse of molecular cloud cores

Min Li and Xiang Li
Monthly Notices of the Royal Astronomical Society 449 (3) 2259 (2015)
https://doi.org/10.1093/mnras/stv435

Delay of planet formation at large radius and the outward decrease in mass and gas content of Jovian planets

Li-Ping Jin, Chun-Jian Liu and Yu Zhang
Research in Astronomy and Astrophysics 15 (9) 1597 (2015)
https://doi.org/10.1088/1674-4527/15/9/015

ZOMBIE VORTEX INSTABILITY. I. A PURELY HYDRODYNAMIC INSTABILITY TO RESURRECT THE DEAD ZONES OF PROTOPLANETARY DISKS

Philip S. Marcus, Suyang Pei, Chung-Hsiang Jiang, et al.
The Astrophysical Journal 808 (1) 87 (2015)
https://doi.org/10.1088/0004-637X/808/1/87

Growth of hydrodynamic perturbations in accretion disks: Possible route to non-magnetic turbulence

Banibrata Mukhopadhyay, Niayesh Afshordi and Ramesh Narayan
Advances in Space Research 38 (12) 2877 (2006)
https://doi.org/10.1016/j.asr.2005.09.048

Blowing in the wind. II. Creation and redistribution of refractory inclusions in a turbulent protoplanetary nebula

Jeffrey N. Cuzzi, Sanford S. Davis and Anthony R. Dobrovolskis
Icarus 166 (2) 385 (2003)
https://doi.org/10.1016/j.icarus.2003.08.016