| 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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