Dust formation and wind acceleration around the aluminum oxide–rich AGB star W Hydrae-Reference-Cited by-同舟云学术

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

Published:2017-11-03 Issue:11 Volume:3 Page:
ISSN:2375-2548
Container-title:Science Advances
language:en
Short-container-title:Sci. Adv.

Author:

Takigawa Aki¹^ORCID,Kamizuka Takafumi²^ORCID,Tachibana Shogo³^ORCID,Yamamura Issei⁴⁵^ORCID

Affiliation:

1. The Hakubi Center for Advanced Research/Division of Earth and Planetary Sciences, Kyoto University, Kitashirakawa Oiwake-cho, Sakyo, Kyoto 606-8502, Japan.

2. Institute of Astronomy, The University of Tokyo, 2-21-1 Osawa, Mitaka, Tokyo 181-0015, Japan.

3. Department of Natural History Science, Hokkaido University, N10W8, Sapporo, Hokkaido 060-0810, Japan.

4. Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, 3-1-1 Yoshinodai, Chuo-ku, Sagamihara, Kanagawa 252-5210, Japan.

5. Department of Space and Astronautical Science, SOKENDAI, 3-1-1 Yoshinodai, Chuo-ku, Sagamihara, Kanagawa 252-5210, Japan.

Abstract

AlO and 29 SiO distributions around W Hya showed that AlO efficiently forms dust and contributes to the wind acceleration.

Funder

Japan Society for the Promotion of Science

Publisher

American Association for the Advancement of Science (AAAS)

Subject

Multidisciplinary

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