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アキタヤ ヒロシ
秋田谷 洋 所属 千葉工業大学 天文学研究センター 天文学研究センター 職種 上席研究員 |
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| 言語種別 | 英語 |
| 発行・発表の年月 | 2021/08/01 |
| 形態種別 | 学術雑誌 |
| 標題 | Origins of the Long-term Variability of the Near-infrared Emission of the Black Hole X-Ray Binary GRS 1915+105 in the X-Ray Low Luminous State |
| 執筆形態 | 共著 |
| 掲載誌名 | The Astrophysical Journal |
| 掲載区分 | 国外 |
| 出版社・発行元 | American Astronomical Society |
| 巻・号・頁 | 916(2),pp.114 |
| 著者・共著者 | Fumiya Imazato, Mahito Sasada, Makoto Uemura, Yasushi Fukazawa, Hiromitsu Takahashi, Tatsuya Nakaoka, Hiroshi Akitaya, Koji S. Kawabata, Masanori Akimoto, Kenta Fujisawa |
| 概要 | Since 2018 July, the black hole X-ray binary GRS 1915+105 has been in an X-ray low luminous state (XLLS), which is the faintest period ever observed in a soft X-ray band. We present here the results of near-infrared (NIR) observations from 2019 April–December in the XLLS using HONIR attached to the Kanata telescope, together with radio data obtained by the Yamaguchi Interferometer and archival X-ray data. We found the historical NIR brightening in the XLLS. |
| DOI | 10.3847/1538-4357/ac07a3 |
| ISSN | 0004637X |
| NAID | 1360857593653603456 |