In this paper we describe the potential of the enhanced X-ray Timing and Polarimetry (eXTP) mission for studies related to accretion flows in the strong field gravity regime around both stellar-mass and supermassive black-holes. eXTP has the unique capability of using advanced “spectral-timing-polarimetry” techniques to analyze the rapid variations with three orthogonal diagnostics of the flow and its geometry, yielding unprecedented insight into the inner accreting regions, the effects of strong field gravity on the material within them and the powerful outflows which are driven by the accretion process. X-spinmeasurements.

Accretion in strong field gravity with eXTP / De Rosa, Alessandra; Uttley, Phil; Gou, Lijun; Liu, Yuan; Bambi, Cosimo; Barret, Didier; Belloni, Tomaso; Berti, Emanuele; Bianchi, Stefano; Caiazzo, Ilaria; Casella, Piergiorgio; Feroci, Marco; Ferrari, Valeria; Gualtieri, Leonardo; Heyl, Jeremy; Ingram, Adam; Karas, Vladimir; Lu, Fangjun; Luo, Bin; Matt, Giorgio; Motta, Sara; Neilsen, Joseph; Pani, Paolo; Santangelo, Andrea; Shu, Xinwen; Wang, Junfeng; Wang, Jian-Min; Xue, Yongquan; Xu, Yupeng; Yuan, Weimin; Yuan, Yefei; Zhang, Shuang-Nan; Zhang, Shu; Agudo, Ivan; Amati, Lorenzo; Andersson, Nils; Baglio, Cristina; Bakala, Pavel; Baykal, Altan; Bhattacharyya, Sudip; Bombaci, Ignazio; Bucciantini, Niccoló; Capitanio, Fiamma; Ciolfi, Riccardo; Cui, Wei K.; D’Ammando, Filippo; Dauser, Thomas; Del Santo, Melania; De Marco, Barbara; Di Salvo, Tiziana; Done, Chris; Dovčiak, Michal; Fabian, Andrew C.; Falanga, Maurizio; Gambino, Angelo Francesco; Gendre, Bruce; Grinberg, Victoria; Heger, Alexander; Homan, Jeroen; Iaria, Rosario; Jiang, Jiachen; Jin, Chichuan; Koerding, Elmar; Linares, Manu; Liu, Zhu; Maccarone, Thomas J.; Malzac, Julien; Manousakis, Antonios; Marin, Frédéric; Marinucci, Andrea; Mehdipour, Missagh; Méndez, Mariano; Migliari, Simone; Miller, Cole; Miniutti, Giovanni; Nardini, Emanuele; O’Brien, Paul T.; Osborne, Julian P.; Petrucci, Pierre Olivier; Possenti, Andrea; Riggio, Alessandro; Rodriguez, Jerome; Sanna, Andrea; Shao, Lijing; Sobolewska, Malgosia; Sramkova, Eva; Stevens, Abigail L.; Stiele, Holger; Stratta, Giulia; Stuchlik, Zdenek; Svoboda, Jiri; Tamburini, Fabrizio; Tauris, Thomas M.; Tombesi, Francesco; Torok, Gabriel; Urbanec, Martin; Vincent, Frederic; Wu, Qingwen; Yuan, Feng; in’ t Zand, Jean J. M.; Zdziarski, Andrzej A.; Zhou, Xinlin. - In: SCIENCE CHINA. PHYSICS, MECHANICS & ASTRONOMY. - ISSN 1674-7348. - 62:2(2019). [10.1007/s11433-018-9297-0]

Accretion in strong field gravity with eXTP

Ferrari, Valeria;Gualtieri, Leonardo;Pani, Paolo;
2019

Abstract

In this paper we describe the potential of the enhanced X-ray Timing and Polarimetry (eXTP) mission for studies related to accretion flows in the strong field gravity regime around both stellar-mass and supermassive black-holes. eXTP has the unique capability of using advanced “spectral-timing-polarimetry” techniques to analyze the rapid variations with three orthogonal diagnostics of the flow and its geometry, yielding unprecedented insight into the inner accreting regions, the effects of strong field gravity on the material within them and the powerful outflows which are driven by the accretion process. X-spinmeasurements.
2019
accretion; black holes physics; X-ray; Physics and Astronomy (all)
01 Pubblicazione su rivista::01a Articolo in rivista
Accretion in strong field gravity with eXTP / De Rosa, Alessandra; Uttley, Phil; Gou, Lijun; Liu, Yuan; Bambi, Cosimo; Barret, Didier; Belloni, Tomaso; Berti, Emanuele; Bianchi, Stefano; Caiazzo, Ilaria; Casella, Piergiorgio; Feroci, Marco; Ferrari, Valeria; Gualtieri, Leonardo; Heyl, Jeremy; Ingram, Adam; Karas, Vladimir; Lu, Fangjun; Luo, Bin; Matt, Giorgio; Motta, Sara; Neilsen, Joseph; Pani, Paolo; Santangelo, Andrea; Shu, Xinwen; Wang, Junfeng; Wang, Jian-Min; Xue, Yongquan; Xu, Yupeng; Yuan, Weimin; Yuan, Yefei; Zhang, Shuang-Nan; Zhang, Shu; Agudo, Ivan; Amati, Lorenzo; Andersson, Nils; Baglio, Cristina; Bakala, Pavel; Baykal, Altan; Bhattacharyya, Sudip; Bombaci, Ignazio; Bucciantini, Niccoló; Capitanio, Fiamma; Ciolfi, Riccardo; Cui, Wei K.; D’Ammando, Filippo; Dauser, Thomas; Del Santo, Melania; De Marco, Barbara; Di Salvo, Tiziana; Done, Chris; Dovčiak, Michal; Fabian, Andrew C.; Falanga, Maurizio; Gambino, Angelo Francesco; Gendre, Bruce; Grinberg, Victoria; Heger, Alexander; Homan, Jeroen; Iaria, Rosario; Jiang, Jiachen; Jin, Chichuan; Koerding, Elmar; Linares, Manu; Liu, Zhu; Maccarone, Thomas J.; Malzac, Julien; Manousakis, Antonios; Marin, Frédéric; Marinucci, Andrea; Mehdipour, Missagh; Méndez, Mariano; Migliari, Simone; Miller, Cole; Miniutti, Giovanni; Nardini, Emanuele; O’Brien, Paul T.; Osborne, Julian P.; Petrucci, Pierre Olivier; Possenti, Andrea; Riggio, Alessandro; Rodriguez, Jerome; Sanna, Andrea; Shao, Lijing; Sobolewska, Malgosia; Sramkova, Eva; Stevens, Abigail L.; Stiele, Holger; Stratta, Giulia; Stuchlik, Zdenek; Svoboda, Jiri; Tamburini, Fabrizio; Tauris, Thomas M.; Tombesi, Francesco; Torok, Gabriel; Urbanec, Martin; Vincent, Frederic; Wu, Qingwen; Yuan, Feng; in’ t Zand, Jean J. M.; Zdziarski, Andrzej A.; Zhou, Xinlin. - In: SCIENCE CHINA. PHYSICS, MECHANICS & ASTRONOMY. - ISSN 1674-7348. - 62:2(2019). [10.1007/s11433-018-9297-0]
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11573/1243180
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