The properties of the clumpy torus and BLR in the polar-scattered Seyfert 1 galaxy ESO 323-G77 through X-ray absorption variability
The properties of the clumpy torus and BLR in the polar-scattered Seyfert 1 galaxy ESO 323-G77 through X-ray absorption variability
复制标题
通过 X 射线吸收变化观察极散射 Seyfert 1 星系 ESO 323-G77 中块状环面和 BLR 的特性
DOI：
10.1093/mnras/stt2005
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发表时间：
2013
影响因子：
4.8
通讯作者：
E. Jiménez
中科院分区：
文献类型：
--
作者：
G. Miniutti;M. Sanfrutos;T. Beuchert;B. Agís;A. Longinotti;E. Piconcelli;Y. Krongold;M. Guainazzi;Stefano Bianchi;G. Matt;E. Jiménez
通用汽车感谢皮拉尔埃斯奎伊和阿尔穆德纳阿隆索-埃雷罗进行了有益的讨论。这项工作是以XMM-牛顿获得的观测结果为基础的，XMM-牛顿是欧空局的一项科学使命，其仪器和捐款由欧空局成员国和美国航天局直接资助。本研究还利用了高能天体物理学科学档案研究中心（HEASARC）提供的数据和/或软件，该中心是NASA/GSFC天体物理科学部和史密森天体物理学部的一个服务部门天体物理天文台。我们利用了从钱德拉数据档案和钱德拉源目录获得的数据，以及钱德拉X射线中心（CXC）提供的软件和从斯威夫特天文台获得的数据。我们还利用了朱雀天文台的数据，这是日本（JAXA）和美国（NASA）航天机构之间的一项合作使命。BAG、GM和MS感谢西班牙MINECO通过AYA 2010 -21490-C 02 -02赠款下的西班牙国家天文学和天体物理计划提供的支持。
GM thanks Pilar Esquej and Almudena Alonso-Herrero for useful discussions. This work is based on observations obtained with XMM–Newton , an ESA science mission with instruments and contributions directly funded by ESA Member States and NASA. This research has also made use of data and/or software provided by the High Energy Astrophysics Science Archive Research Center (HEASARC), which is a service of the Astrophysics Science Division at NASA/GSFC and the High Energy Astrophysics Division of the Smithsonian Astrophysical Observatory. We made use of data obtained from the Chandra Data Archive and the Chandra Source Catalogue, and software provided by the Chandra X-ray Center (CXC) and of data obtained from the Swift observatory. We also made use of data from the Suzaku observatory, a collaborative mission between the space agencies of Japan (JAXA) and the USA (NASA). BAG, GM and MS thank the Spanish MINECO for support through the Spanish Plan Nacional de Astronomia y Astrofisica under grant AYA2010-21490-C02-02.