Accretion in strong field gravity with eXTP

Journal
SCIENCE CHINA. PHYSICS, MECHANICS & ASTRONOMY
Date Issued
2019
Author(s)
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Uttley, Phil
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Gou, LiJun
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Liu, Yuan
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Bambi, Cosimo
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Barret, Didier
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Berti, Emanuele
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BIANCHI, STEFANO
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Caiazzo, Ilaria
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Yuan, Feng
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in't Zand, Jean J. M.
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Zdziarski, Andrzej A.
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Zhou, XinLin
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Ferrari, Valeria
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Gualtieri, Leonardo
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Heyl, Jeremy
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Ingram, Adam
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Karas, Vladimir
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Lu, FangJun
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Luo, Bin
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Neilsen, Joseph
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Pani, Paolo
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Santangelo, Andrea
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Shu, XinWen
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Wang, JunFeng
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Wang, Jian-Min
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Xue, YongQuan
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Xu, YuPeng
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Yuan, WeiMin
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Yuan, YeFei
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Zhang, Shuang-Nan
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Zhang, Shu
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Agudo, Ivan
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Andersson, Nils
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Baglio, Cristina
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Bakala, Pavel
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Baykal, Altan
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Bhattacharyya, Sudip
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Bombaci, Ignazio
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Cui, Wei K.
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Dauser, Thomas
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De Marco, Barbara
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Done, Chris
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Dovčiak, Michal
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Fabian, Andrew C.
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Falanga, Maurizio
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Gambino, Angelo Francesco
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Gendre, Bruce
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Grinberg, Victoria
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Heger, Alexander
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Homan, Jeroen
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Jiang, JiaChen
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Jin, ChiChuan
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Koerding, Elmar
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Linares, Manu
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Liu, Zhu
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Maccarone, Thomas J.
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Malzac, Julien
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Manousakis, Antonios
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Marin, Frédéric
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Marinucci, Andrea
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Mehdipour, Missagh
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Méndez, Mariano
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Migliari, Simone
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Miller, Cole
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Miniutti, Giovanni
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O'Brien, Paul T.
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Osborne, Julian P.
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Petrucci, Pierre Olivier
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Rodriguez, Jerome
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Shao, LiJing
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Sobolewska, Malgosia
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Sramkova, Eva
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Stevens, Abigail L.
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Stiele, Holger
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Stuchlik, Zdenek
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Svoboda, Jiri
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Tamburini, Fabrizio
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Tauris, Thomas M.
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Torok, Gabriel
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Urbanec, Martin
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Vincent, Frederic
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Wu, QingWen
DOI
10.1007/s11433-018-9297-0
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
Volume
62
Issue
2
Start page
29504
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