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Variability of the warm absorber in the low-mass X-ray binary GX 13+1 with XMM-Newton
https://jaxa.repo.nii.ac.jp/records/5033
https://jaxa.repo.nii.ac.jp/records/5033e082d76b-a573-4b23-ad7e-d68aabb0d3c4
名前 / ファイル | ライセンス | アクション |
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64574101.pdf (186.2 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 | Variability of the warm absorber in the low-mass X-ray binary GX 13+1 with XMM-Newton | |||||
言語 | ||||||
言語 | eng | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | Accretion, accretion discs - X-rays: individual: GX 13+1 | |||||
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 |
Diaz, Trigo Maria
× Diaz, Trigo Maria× Sidoli, L.× Parmar, A.× Boirin, L. |
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著者所属(英) | ||||||
en | ||||||
ESAC | ||||||
著者所属(英) | ||||||
en | ||||||
INAF, IASF | ||||||
著者所属(英) | ||||||
en | ||||||
ESAC | ||||||
著者所属(英) | ||||||
en | ||||||
Observatoire Astronomique de Strasbourg | ||||||
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. 276-277, 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 have analysed data from five XMM-Newton observations of GX 13+1, to investigate the variability of the photo-ionised absorber present in this source. We fit the EPIC spectra obtained from "persistent" (non-variable) intervals with a model consisting of disc-blackbody and blackbody components together with a Gaussian emission feature at approximately 6.6 keV modified by absorption due to cold and photo-ionised material. Observations with a hard spectrum, with high temperatures for the blackbody (kT approximately 1.6 keV) and disc blackbody (kT approximately 1.1 keV) show a very ionised absorber with absorption due to FeXXVI and a modest emission Gaussian, with an equivalent width of 70 eV. In contrast, observations with softer spectra, with a colder blackbody (kT approximately 1.2 keV) and disc blackbody (kT approximately 0.75 keV) show a cooler absorber, with FeXXV and FeXXVI features, and a stronger emission Gaussian, with an equivalent width of approximately 180 eV. This analysis reveals a direct relation between the continuum emission, the ionisation state of outflow and the strength and ionisation of the iron emission line. | |||||
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: AA0064574101 | |||||
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 |