Dependence of Hall coefficient on grain size and cosmic ray rate and implication for circumstellar disc formation-Reference-Cited by-同舟云学术

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Dependence of Hall coefficient on grain size and cosmic ray rate and implication for circumstellar disc formation

Published:2019-01-02 Issue:2 Volume:484 Page:2119-2136
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Koga Shunta¹,Tsukamoto Yusuke²,Okuzumi Satoshi³,Machida Masahiro N¹

Affiliation:

1. Department of Earth and Planetary Sciences, Faculty of Sciences, Kyushu University, Fukuoka 819-0395, Japan

2. Department of Earth and Space Science, Graduate Schools of Science and Engineering, Kagoshima University, Kagoshima 890-0065, Japan

3. Department of Earth and Planetary Sciences, Tokyo Institute of Technology, Tokyo 152-8551, Japan

Funder

Japan Society for the Promotion of Science

Japan Agency for Marine-Earth Science and Technology

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/484/2/2119/27620629/sty3524.pdf

Reference63 articles.

1. From T Tauri stars to protostars: Circumstellar material and young stellar objects in the rho Ophiuchi cloud

2. Hall Effect–Mediated Magnetic Flux Transport in Protoplanetary Disks

3. Collapse of a Molecular Cloud Core to Stellar Densities: The First Three-dimensional Calculations

4. The Hall effect in star formation

5. Dense Cores in Dark Clouds. XIV. N2H+(1–0) Maps of Dense Cloud Cores

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1. Magnetohydrodynamical modeling of star-disk formation: from isolated spherical collapse towards incorporation of external dynamics;Frontiers in Astronomy and Space Sciences;2024-08-28

2. The First Estimation of the Ambipolar Diffusivity Coefficient from Multi-scale Observations of the Class 0/I Protostar, HOPS-370;The Astrophysical Journal;2024-06-01

3. Formation of Unipolar Outflow and Protostellar Rocket Effect in Magnetized Turbulent Molecular Cloud Cores;The Astrophysical Journal;2024-02-23

4. Impact of turbulence intensity and fragmentation velocity on dust particle size evolution and non-ideal magnetohydrodynamics effects;Monthly Notices of the Royal Astronomical Society;2023-04-27

5. Dust motion and possibility of dust growth in a growing circumstellar disk;Monthly Notices of the Royal Astronomical Society;2022-12-02

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