Settling time of solid grains in gaseous giant protoplanets-Reference-Cited by-同舟云学术

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Settling time of solid grains in gaseous giant protoplanets

Published:2021-06 Issue: Volume:200 Page:105212
ISSN:0032-0633
Container-title:Planetary and Space Science
language:en
Short-container-title:Planetary and Space Science

Author:

Chandra Paul Gour,Bilkis Farjana,Ali Md Emran,Chandra Barman Mrinal

Funder

National Science and Technology Planning Project

Queen Mary University of London

Publisher

Elsevier BV

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference69 articles.

1. Ringed substructure and a gap at 1 au in the nearest protoplanetary disk;Andrews;Astrophys. J.,2016

2. The disk substructures at high angular resolution project (DSHARP). I. Motivation, sample, calibration, and overview;Andrews;Astrophys. J.,2018

3. Growth of interstellar grains;Baines;Nature (London),1965

4. Gas and dust evolution in protoplanetary disks;Birnstiel;Astron. Astrophys.,2010

5. Calculations of the evolution of the giant planets;Bodenheimer;Icarus,1980

Cited by 4 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. Unveiling protoplanetary structure equations: Semi-analytical solutions via the homotopy analysis method;Heliyon;2024-08

2. On the radius spectrum of solid grains settling in polytropic protoplanets;The European Physical Journal Plus;2024-07-10

3. An effective method in investigating structures of polytropic protoplanets formed via gravitational instability;Heliyon;2022-09

4. Solving protoplanetary structure equations using Adomian decomposition method;Heliyon;2021-10

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