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Rotation in the NGC 1333 IRAS 4C Outflow
http://hdl.handle.net/2241/00153584
http://hdl.handle.net/2241/0015358464cb3db4-b341-4c57-9b5f-5a126efc3f01
| 名前 / ファイル | ライセンス | アクション |
|---|---|---|
ApJ_864-1-76.pdf (2.6 MB)
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| Item type | Journal Article(1) | |||||
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| 公開日 | 2018-10-22 | |||||
| タイトル | ||||||
| タイトル | Rotation in the NGC 1333 IRAS 4C Outflow | |||||
| 言語 | en | |||||
| 言語 | ||||||
| 言語 | eng | |||||
| 資源タイプ | ||||||
| 資源タイプ識別子 | http://purl.org/coar/resource_type/c_6501 | |||||
| 資源タイプ | journal article | |||||
| アクセス権 | ||||||
| アクセス権 | open access | |||||
| アクセス権URI | http://purl.org/coar/access_right/c_abf2 | |||||
| 著者 |
Zhang, Yichen
× Zhang, Yichen× Higuchi, Aya E.× Sakai, Nami× Oya, Yoko× Lopez-Sepulcre, Ana× Imai, Muneaki× Sakai, Takeshi× 渡邉, 祥正× Ceccarelli, Cecilia× Lefloch, Bertrand× Yamamoto, Satoshi |
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| 抄録 | ||||||
| 内容記述タイプ | Abstract | |||||
| 内容記述 | We report molecular line observations of the NGC 1333 IRAS 4C outflow in the Perseus Molecular Cloud with the Atacama Large Millimeter/Submillimeter Array. The CCH and CS emission reveal an outflow cavity structure with clear signatures of rotation with respect to the outflow axis. The rotation is detected from about 120 au up to about 1400 au above the envelope/disk midplane. As the distance to the central source increases, the rotation velocity of the outflow decreases while the outflow radius increases, which gives a flat specific angular momentum distribution along the outflow. The mean specific angular momentum of the outflow is about 100 au km s-1. On the basis of reasonable assumptions on the outward velocity of the outflow and the protostar mass, we estimate the range of outflow-launching radii to be 5–15 au. Such a launching radius rules out that this outflow is launched as an X-wind, but rather, it is more consistent to be a slow disk wind launched from relatively large radii on the disk. The radius of the centrifugal barrier is roughly estimated, and the role of the centrifugal barrier in the outflow launching is discussed. | |||||
| 言語 | en | |||||
| 書誌情報 |
en : The Astrophysical journal 巻 864, 号 1, p. 76, 発行日 2018-08 |
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| ISSN | ||||||
| 収録物識別子タイプ | PISSN | |||||
| 収録物識別子 | 1538-4365 | |||||
| NCID | ||||||
| 収録物識別子タイプ | NCID | |||||
| 収録物識別子 | AA00553253 | |||||
| DOI | ||||||
| 関連タイプ | isIdenticalTo | |||||
| 識別子タイプ | DOI | |||||
| 関連識別子 | https://doi.org/10.3847/1538-4357/aad7ba | |||||
| 権利情報 | ||||||
| 言語 | en | |||||
| 権利情報 | © 2018. The American Astronomical Society. | |||||
| 権利情報 | ||||||
| 言語 | en | |||||
| 権利情報 | Original content from this work may be used under the terms of the Creative Commons Attribution 3.0 licence. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI. | |||||
| 出版タイプ | ||||||
| 出版タイプ | VoR | |||||
| 出版タイプResource | http://purl.org/coar/version/c_970fb48d4fbd8a85 | |||||
| 出版者 | ||||||
| 出版者 | IOP Publishing | |||||
| 言語 | en | |||||
