Research ArticleASTRONOMY

Dust formation and wind acceleration around the aluminum oxide–rich AGB star W Hydrae

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Science Advances  01 Nov 2017:
Vol. 3, no. 11, eaao2149
DOI: 10.1126/sciadv.aao2149

Article Information

vol. 3 no. 11

Online ISSN: 
History: 
  • Received for publication June 26, 2017
  • Accepted for publication October 4, 2017

Author Information

  1. Aki Takigawa1,*,
  2. Takafumi Kamizuka2,
  3. Shogo Tachibana3, and
  4. Issei Yamamura4,5
  1. 1The Hakubi Center for Advanced Research/Division of Earth and Planetary Sciences, Kyoto University, Kitashirakawa Oiwake-cho, Sakyo, Kyoto 606-8502, Japan.
  2. 2Institute of Astronomy, The University of Tokyo, 2-21-1 Osawa, Mitaka, Tokyo 181-0015, Japan.
  3. 3Department of Natural History Science, Hokkaido University, N10W8, Sapporo, Hokkaido 060-0810, Japan.
  4. 4Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, 3-1-1 Yoshinodai, Chuo-ku, Sagamihara, Kanagawa 252-5210, Japan.
  5. 5Department of Space and Astronautical Science, SOKENDAI, 3-1-1 Yoshinodai, Chuo-ku, Sagamihara, Kanagawa 252-5210, Japan.
  1. *Corresponding author. Email: takigawa{at}kueps.kyoto-u.ac.jp
  • Present address: UTokyo Organization for Planetary and Space Science/Department of Earth and Planetary Science, The University of Tokyo, 7-3-1 Hongo, Tokyo 113-0033, Japan.

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