Radiation-pressure-driven dust transport to galaxy haloes at z ∼ 10-Reference-Cited by-同舟云学术

Radiation-pressure-driven dust transport to galaxy haloes at z ∼ 10

Published:2019-05-16 Issue:1 Volume:487 Page:961-974
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Hirashita Hiroyuki¹,Inoue Akio K²³⁴^ORCID

Affiliation:

1. Institute of Astronomy and Astrophysics, Academia Sinica, Astronomy-Mathematics Building, AS/NTU, No. 1, Sec. 4, Roosevelt Road, Taipei 10617, Taiwan

2. Department of Environmental Science and Technology, Faculty of Design Technology, Osaka Sangyo University, 3-1-1, Nakagaito, Daito, Osaka 574-8530, Japan

3. Department of Physics, School of Advanced Science and Engineering, Waseda University, 3-4-1, Okubo, Shinjuku, Tokyo 169-8555, Japan

4. Waseda Research Institute for Science and Engineering, 3-4-1, Okubo, Shinjuku, Tokyo 169-8555, Japan

Funder

Ministry of Science and Technology

National Astronomical Observatory of Japan

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/advance-article-pdf/doi/10.1093/mnras/stz1348/28656779/stz1348.pdf

Reference74 articles.

1. Dust versus Cosmic Acceleration

2. Dust dynamics and evolution in expanding H ii regions. I. Radiative drift of neutral and charged grains

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5. Galaxy simulation with dust formation and destruction

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