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Fe -K line Profile and X-ray Spectral Variability of the Seyfert 1.9 Galaxy NGC 7314 Observed with Suzaku
https://jaxa.repo.nii.ac.jp/records/5057
https://jaxa.repo.nii.ac.jp/records/50574436c2a7-09a0-4531-b8de-5e2772004472
名前 / ファイル | ライセンス | アクション |
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64574125.pdf (218.7 kB)
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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 | Fe -K line Profile and X-ray Spectral Variability of the Seyfert 1.9 Galaxy NGC 7314 Observed with Suzaku | |||||
言語 | ||||||
言語 | eng | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | Seyfert galaxy, NGC 7314, variability | |||||
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 |
河原, 大
× 河原, 大× 寺島, 雄一× 粟木, 久光× Kawahara, Hiroshi× Terashima, Yuichi× Yaqoob, Tahir× Awaki, Hisamitsu |
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著者所属 | ||||||
愛媛大学 | ||||||
著者所属 | ||||||
愛媛大学 | ||||||
著者所属 | ||||||
愛媛大学 | ||||||
著者所属(英) | ||||||
en | ||||||
Ehime University | ||||||
著者所属(英) | ||||||
en | ||||||
Ehime University | ||||||
著者所属(英) | ||||||
en | ||||||
Johns Hopkins University | ||||||
著者所属(英) | ||||||
en | ||||||
Ehime University | ||||||
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: The Energetic Cosmos; from Suzaku to ASTRO-H 巻 JAXA-SP-09-008E, p. 324-325, 発行日 2010-02-26 |
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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 | The 3rd Suzaku international Conference "Energetic Cosmos : from Suzaku to ASTRO-H" (June 29-July 2, 2009. Grand Park Otaru Hotel), Otaru, Hokkaido Japan | |||||
抄録(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | We present results from a Suzaku observation of the Seyfert 1.9 galaxy NGC 7314. The light curve in the 2-10 keV band shows rapid variability on timescales of approximately 1000 sec. The time-averaged spectrum in 0.5 - 25 keV is explained a model consisting of absorbed and unabsorbed power laws, a reflection continuum and a gaussian at 6.4 keV. The line at 6.4 keV is relatively narrow (sigma approximately 50 eV) and does not vary on a timescale of approximately 10 years. This narrow line is likely to be primarily from distant matter. We analyze spectra in the time intervals with fluxes higher/lower than the mean. The normalization of the absorbed power law varies by a factor 1.6, while the photon index, the amount of the reflection, and the intensity of the Fe line remains constant. | |||||
内容記述(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | Meeting sponsors: The University of Tokyo, The Institute of Physical and Chemical Research, The Japan Society for the Promotion of Science | |||||
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: AA0064574125 | |||||
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-09-008E |