Effect of dust size and structure on scattered-light images of protoplanetary discs-Reference-Cited by-同舟云学术

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Effect of dust size and structure on scattered-light images of protoplanetary discs

Published:2019-03-08 Issue:4 Volume:485 Page:4951-4966
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Tazaki Ryo¹^ORCID,Tanaka H¹,Muto T²,Kataoka A³^ORCID,Okuzumi S⁴

Affiliation:

1. Astronomical Institute, Graduate School of Science, Tohoku University, 6-3 Aramaki, Aoba-ku, Sendai 980-8578, Japan

2. Division of Liberal Arts, Kogakuin University, 1-24-2 Nishi-Shinjuku, Shinjuku-ku, Tokyo 163-8677, Japan

3. National Astronomical Observatory of Japan, Mitaka, Tokyo 181-8588, Japan

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

Funder

Japan Society for the Promotion of Science

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/485/4/4951/28249824/stz662.pdf

Reference61 articles.

1. STRUCTURES IN THE PROTOPLANETARY DISK OF HD142527 SEEN IN POLARIZED SCATTERED LIGHT

2. Disks around T Tauri Stars with SPHERE (DARTTS-S). I. SPHERE/IRDIS Polarimetric Imaging of Eight Prominent T Tauri Disks

3. Aggregate dust particles at comet 67P/Churyumov–Gerasimenko

4. Optics of Fractal Clusters Such as Smoke

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