Circumstellar disks of the most vigorously accreting young stars-Reference-Cited by-同舟云学术

Circumstellar disks of the most vigorously accreting young stars

Published:2016-02-05 Issue:2 Volume:2 Page:
ISSN:2375-2548
Container-title:Science Advances
language:en
Short-container-title:Sci. Adv.

Author:

Liu Hauyu Baobab¹,Takami Michihiro¹^ORCID,Kudo Tomoyuki²,Hashimoto Jun²,Dong Ruobing¹³,Vorobyov Eduard I.⁴⁵,Pyo Tae-Soo²,Fukagawa Misato²,Tamura Motohide²⁶,Henning Thomas⁷^ORCID,Dunham Michael M.⁸,Karr Jennifer L.¹^ORCID,Kusakabe Nobuhiko²,Tsuribe Toru⁹

Affiliation:

1. Academia Sinica Institute of Astronomy and Astrophysics, Taipei 10617, Taiwan.

2. National Astronomical Observatory of Japan, Tokyo 181-8588, Japan.

3. Astronomy Department, University of California Berkeley, Berkeley, CA 94720, USA.

4. Department of Astrophysics, University of Vienna, Vienna 1010, Austria.

5. Research Institute of Physics, Southern Federal University, Rostov-on-Don 344006, Russia.

6. University of Tokyo, Tokyo 113-8654, Japan.

7. Max-Planck-Institut für Astronomie, Heidelberg 69117, Germany.

8. Harvard-Smithsonian Center for Astrophysics, Cambridge, MA 02138, USA.

9. College of Science, Ibaraki University, Mito 310-0056, Japan.

Abstract

Subaru-HiCIAO observations on FU Orionis objects revealed asymmetric structures on 10 2 to 10 3 AU scales of circumstellar disks and envelopes.

Publisher

American Association for the Advancement of Science (AAAS)

Subject

Multidisciplinary

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