A dynamic black hole corona in an active galaxy through X-ray reverberation mapping

A dynamic black hole corona in an active galaxy through X-ray reverberation mapping

X-ray reverberation echoes are assumed to be produced in the strongly distorted spacetime around accreting supermassive black holes. This signal allows us to spatially map the geometry of the inner accretion flow1,2—a region that cannot yet be spatially resolved by any telescope—and provides a direc...

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書誌詳細
主要な著者: Alston, William N., Fabian, Andrew C., Kara, Erin A, Parker, Michael L., Dovciak, Michal, Pinto, Ciro, Jiang, Jiachen, Middleton, Matthew J., Miniutti, Giovanni, Walton, Dominic J., Wilkins, Dan R., Buisson, Douglas J. K., Caballero-Garcia, Maria D., Cackett, Edward M., De Marco, Barbara, Gallo, Luigi C., Lohfink, Anne M., Reynolds, Chris S., Uttley, Phil, Young, Andrew J., Zogbhi, Abderahmen
その他の著者: MIT Kavli Institute for Astrophysics and Space Research
フォーマット: 論文
言語:English
出版事項: Springer Science and Business Media LLC 2021
オンライン･アクセス:https://hdl.handle.net/1721.1/129519

インターネット

https://hdl.handle.net/1721.1/129519

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