言語種別 | 日本語 |
発行・発表の年月 | 2020/03 |
形態種別 | 学術雑誌 |
査読 | 査読あり |
標題 | Sub-millimeter detection of a Galactic center cool star IRS 7 by ALMA
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執筆形態 | 共著 |
掲載誌名 | Publications of the Astronomical Society of Japan |
掲載区分 | 国内 |
担当範囲 | データ解析,議論 |
著者・共著者 | Masato Tsuboi, Yoshimi Kitamura, Takahiro Tsutsumi, Ryosuke Miyawaki, Makoto Miyoshi, Atsushi Miyazaki
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概要 | IRS 7 is an M red supergiant star which is located at 5′′.5 north of Sagittarius A∗. We detected firstly the continuum emission at 340GHz of IRS 7 using the Atacama Large Millimeter/submillimeter Array (ALMA). The total flux density of IRS 7 is Sν=448±45μJy. The flux density indicates that IRS 7 has a photosphere radius of R=1170±60R⊙, which is roughly consistent with the previous Very Large Telescope Interferometer measurement. We also detected a shell-like feature with a northern extension in the H30α recombination line using ALMA. |
researchmap用URL | https://doi.org/10.1093/pasj/psaa013 |
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