Please use this identifier to cite or link to this item: http://hdl.handle.net/20.500.12666/471
Title: Accretion in strong field gravity with eXTP
Authors: De Rosa, A.
Uttley, P.
Gou, L.
Liu, Y.
Bambi, C.
Barret, D.
Belloni, T.
Berti, E.
Bianchi, S.
Caiazzo, I.
Casella, P.
Jiang, J.
Jin, C. C.
Koerding, E.
Linares, M.
Liu, Z.
Maccarone, T. J.
Malzac, J.
Manousakis, A.
Marin, F.
Marinucci, A.
Mehdipour, M.
Méndez, M.
Migliari, S.
Miller, C.
Miniutti, G.
Nardini, E.
O´Brien, P. T.
Osborne, J. P.
Petrucci, P. O.
Possenti, A.
Riggio, A.
Rodríguez, J.
Sanna, A.
Shao, L. J.
Sobolewska, M.
Sramkova, E.
Stevens, A. L.
Stiele, H.
Stratta, G.
Stuchlik, Z.
Svoboda, J.
Tamburini, F.
Tauris, T. M.
Tombesi, F.
Torok, G.
Urbanec, M.
Vicent, F.
Wu, Q. W.
Yuan, F.
Zand, J. J. M.
Zdziarski, A. A.
Zhou, X.
Feroci, M.
Ferrari, V.
Gualtieri, L.
Heyl, J.
Ingram, A.
Karas, V.
Lu, F. J.
Luo, B.
Matt, G.
Motta, S. E.
Neilsen, J.
Pani, P.
Santangelo, A.
Shu, X. W.
Wang, J. F.
Wang, J. M.
Xue, Y. Q.
Xu, Y. P.
Yuan, W. M.
Yuan, Y. F.
Zhang, S. N.
Zhang, S.
Agudo, I.
Amati, L.
Andersson, N. A.
Baglio, C.
Bakala, P.
Baykal, A.
Bhattacharyya, S.
Bombaci, I.
Bucciantini, N.
Capitanio, F.
Ciolfi, R.
Cui, W. K.
D´Ammando, F.
Dauser, T.
Del Santo, M.
De Marco, B.
Di Salvo, T.
Done, C.
Dovciak, M.
Fabian, A. C.
Falanga, M.
Gambino, A. F.
Gendre, B.
Grinberg, V.
Heger, A.
Homan, J.
Iaria, R.
Keywords: X ray;Black holes physics;Accretion
Issue Date: 7-Dec-2018
Publisher: Springer Link
DOI: 10.1007/s11433-018-9297-0
Published version: https://link.springer.com/article/10.1007%2Fs11433-018-9297-0
Citation: Science China Physics, Mechanics & Astronomy 62(2): A029504(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
URI: http://hdl.handle.net/20.500.12666/471
E-ISSN: 1869-1927
ISSN: 1674-7348
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