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Discovery of Decimeter Radio Wave Pulses from Super Massive Black Holes in the Center Region of Our Galaxy : First Preliminary Results
https://doi.org/10.57375/00000736
https://doi.org/10.57375/00000736739fcf5a-c29b-4238-bc27-1dfc1f5f9410
| 名前 / ファイル | ライセンス | アクション |
|---|---|---|
KJ00004437943.pdf (637.1 kB)
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| Item type | 紀要論文 / Departmental Bulletin Paper(1) | |||||
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| 公開日 | 2009-04-04 | |||||
| タイトル | ||||||
| タイトル | Discovery of Decimeter Radio Wave Pulses from Super Massive Black Holes in the Center Region of Our Galaxy : First Preliminary Results | |||||
| 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 | departmental bulletin paper | |||||
| ID登録 | ||||||
| ID登録 | 10.57375/00000736 | |||||
| ID登録タイプ | JaLC | |||||
| 著者 |
Oya, Hiroshi
× Oya, Hiroshi |
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| 抄録 | ||||||
| 内容記述タイプ | Abstract | |||||
| 内容記述 | Pulses of decimeter wavelength radio waves, in the frequency bands of 1.4GHz and 1.6GHz, arriving from the center part of our Galaxy have been discovered by observations made from July 25 to August 26,2005 at Awara Space and Cosmic Radio wave Observatory of Space Communication Science and Technology in Fukui University of Technology, The identified pulse periods are 129.99, 104.55 and 52.003 sec which correspond, respectively to Gaa, Gab, and Gac that had been already detected in decameter wavelength range. Because the decameter wave pulses have been considered to be from the rotating super massive black holes, the origins of decimeter radio pulses detected in the present study can also be considered to be radiated from the same black holes in the center part of our Galaxy. | |||||
| 書誌情報 |
福井工業大学研究紀要. 第一部 号 36, p. 221-228, 発行日 2006-03-18 |
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| 出版者 | ||||||
| 出版者 | 福井工業大学 | |||||
| ISSN | ||||||
| 収録物識別子タイプ | ISSN | |||||
| 収録物識別子 | 2868571 | |||||
| 書誌レコードID | ||||||
| 識別子タイプ | NCID | |||||
| 関連識別子 | TF00009195 | |||||
| 著者版フラグ | ||||||
| 出版タイプ | VoR | |||||
| 出版タイプResource | http://purl.org/coar/version/c_970fb48d4fbd8a85 | |||||
