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Quasi-periodic osicllations and variable emissions In magnetohydrodynamic accretion flows
https://jaxa.repo.nii.ac.jp/records/5266
https://jaxa.repo.nii.ac.jp/records/52665e1b3c5e-f9d1-4978-94fe-4f3b2e1a5a27
名前 / ファイル | ライセンス | アクション |
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64306027.pdf (2.3 MB)
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Item type | 会議発表論文 / Conference Paper(1) | |||||
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公開日 | 2015-03-26 | |||||
タイトル | ||||||
言語 | en | |||||
タイトル | Quasi-periodic osicllations and variable emissions In magnetohydrodynamic accretion flows | |||||
言語 | ||||||
言語 | eng | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | accretion, accretion disks - magnetohydrodynamics : MHD - quasi-periodic oscillations - radiation : radiative transfer | |||||
資源タイプ | ||||||
資源タイプ識別子 | http://purl.org/coar/resource_type/c_5794 | |||||
資源タイプ | conference paper | |||||
著者 |
加藤, 成晃
× 加藤, 成晃× Kato, Yoshiaki |
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著者所属 | ||||||
宇宙航空研究開発機構宇宙科学研究本部 | ||||||
著者所属(英) | ||||||
en | ||||||
Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (ISAS)(JAXA) | ||||||
出版者 | ||||||
出版者 | 宇宙航空研究開発機構 | |||||
出版者(英) | ||||||
出版者 | Japan Aerospace Exploration Agency (JAXA) | |||||
書誌情報 |
宇宙航空研究開発機構特別資料 en : JAXA Special Publication: Astrophysics with All-Sky X-Ray observations: 3rd International MAXI Workshop 巻 JAXA-SP-08-014E, p. 132-134, 発行日 2009-02-27 |
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会議概要(会議名, 開催地, 会期, 主催者等)(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | Astrophysics with All-Sky X-Ray observations: 3rd International MAXI Workshop (RIKEN, 10-12 June 2008) | |||||
抄録(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | We present our study of oscillations and emissions in three-dimensional (3-D) magnetohydrodynamic (MHO) accretion flows around black holes. It is found that a pair of persistent quasi-periodic oscillations (twin QPOs) is excited at the resonant radius, where the ratio of Keplerian frequency to epicyclic frequency is close to 2:1. The power spectrum density (PSD) shows that the lower peak frequency corresponds to the Keplerian frequency, while the upper peak frequency corresponds to the sum of Keplerian frequency and epicyclic frequency. The results provide the first direct evidence for the excitation of resonant disk oscillation in MHD accretion flows. It is also found that the emergent spectra from radio to gamma-ray of the MHD accretion flows fluctuates in the wide range of frequency and does not always vary coherently. | |||||
ISSN | ||||||
収録物識別子タイプ | ISSN | |||||
収録物識別子 | 1349-113X | |||||
書誌レコードID | ||||||
収録物識別子タイプ | NCID | |||||
収録物識別子 | AA11984031 | |||||
資料番号 | ||||||
内容記述タイプ | Other | |||||
内容記述 | 資料番号: AA0064306027 | |||||
レポート番号 | ||||||
内容記述タイプ | Other | |||||
内容記述 | レポート番号: JAXA-SP-08-014E |