Accretion of dust by chondrules in a MHD-turbulent solar nebula-Reference-Cited by-同舟云学术

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Accretion of dust by chondrules in a MHD-turbulent solar nebula

Published:2011-01 Issue:1 Volume:211 Page:876-884
ISSN:0019-1035
Container-title:Icarus
language:en
Short-container-title:Icarus

Author:

Carballido Augusto

Publisher

Elsevier BV

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference37 articles.

1. Astrophysics of Planet Formation;Armitage,2010

2. Balbus, S.A., 2009. Magnetohydrodynamics of protostellar disks. arXiv:0906.0854.

3. Instability, turbulence, and enhanced transport in accretion disks;Balbus;Rev. Mod. Phys.,1998

4. Kinematics of solid particles in a turbulent protoplanetary disc;Carballido;Mon. Not. R. Astron. Soc.,2008

5. Relative velocities of solids in a turbulent protoplanetary disc;Carballido;Mon. Not. R. Astron. Soc.,2010

Cited by 13 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. The Aguas Zarcas carbonaceous chondrite meteorite: Brecciation and aqueous alteration on the parent body;Meteoritics & Planetary Science;2024-05-29

2. Mechanical Modification of Chondrule Fine-grained Rims by Dusty Nebular Shocks;The Planetary Science Journal;2023-06-01

3. Modeling Chondrule Dust Rim Growth with Ellipsoidal Monomers;The Astrophysical Journal;2023-06-01

4. Dependence of the initial internal structure of chondrule rim on dust size distribution;Icarus;2022-03

5. Formation of rims around chondrules via porous aggregate accretion;Icarus;2021-10

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