Accretion in strong field gravity with eXTP

Alessandra De Rosa; Phil Uttley; Li Jun Gou; Yuan Liu; Cosimo Bambi; Didier Barret; Tomaso Belloni; Emanuele Berti; Stefano Bianchi; Ilaria Caiazzo; Piergiorgio Casella; Marco Feroci; Valeria Ferrari; Leonardo Gualtieri; Jeremy Heyl; Adam Ingram; Vladimir Karas; Fang Jun Lu; Bin Luo; Giorgio Matt; Sara Motta; Joseph Neilsen; Paolo Pani; Andrea Santangelo; Xin Wen Shu; Jun Feng Wang; Jian Min Wang; Yong Quan Xue; Yu Peng Xu; Wei Min Yuan; Ye Fei Yuan; Shuang Nan Zhang; Shu Zhang; Ivan Agudo; Lorenzo Amati; Nils Andersson; Cristina Baglio; Pavel Bakala; Altan Baykal; Sudip Bhattacharyya; Ignazio Bombaci; Niccoló Bucciantini; Fiamma Capitanio; Riccardo Ciolfi; Wei K. Cui; Filippo D’Ammando; Thomas Dauser; Melania Del Santo; Barbara De Marco; Tiziana Di Salvo; Chris Done; Michal Dovčiak; Andrew C. Fabian; Maurizio Falanga; Angelo Francesco Gambino; Bruce Gendre; Victoria Grinberg; Alexander Heger; Jeroen Homan; Rosario Iaria; Jia Chen Jiang; Chi Chuan Jin; Elmar Koerding; Manu Linares; Zhu Liu; Thomas J. Maccarone; Julien Malzac; Antonios Manousakis; Frédéric Marin; Andrea Marinucci; Missagh Mehdipour; Mariano Méndez; Simone Migliari; Cole Miller; Giovanni Miniutti; Emanuele Nardini; Paul T. O’Brien; Julian P. Osborne; Pierre Olivier Petrucci; Andrea Possenti; Alessandro Riggio; Jerome Rodriguez; Andrea Sanna; Li Jing Shao; Malgosia Sobolewska; Eva Sramkova; Abigail L. Stevens; Holger Stiele; Giulia Stratta; Zdenek Stuchlik; Jiri Svoboda; Fabrizio Tamburini; Thomas M. Tauris; Francesco Tombesi; Gabriel Torok; Martin Urbanec; Frederic Vincent; Qing Wen Wu; Feng Yuan; Jean J.M. in’ t Zand; Andrzej A. Zdziarski; Xin Lin Zhou

doi:10.1007/s11433-018-9297-0

Accretion in strong field gravity with eXTP

Alessandra De Rosa, Phil Uttley, Li Jun Gou, Yuan Liu, Cosimo Bambi, Didier Barret, Tomaso Belloni, Emanuele Berti, Stefano Bianchi, Ilaria Caiazzo, Piergiorgio Casella, Marco Feroci, Valeria Ferrari, Leonardo Gualtieri, Jeremy Heyl, Adam Ingram, Vladimir Karas, Fang Jun Lu, Bin Luo, Giorgio MattSara Motta, Joseph Neilsen, Paolo Pani, Andrea Santangelo, Xin Wen Shu, Jun Feng Wang, Jian Min Wang, Yong Quan Xue, Yu Peng Xu, Wei Min Yuan, Ye Fei Yuan, Shuang Nan Zhang, Shu Zhang, Ivan Agudo, Lorenzo Amati, Nils Andersson, Cristina Baglio, Pavel Bakala, Altan Baykal, Sudip Bhattacharyya, Ignazio Bombaci, Niccoló Bucciantini, Fiamma Capitanio, Riccardo Ciolfi, Wei K. Cui, Filippo D’Ammando, Thomas Dauser, Melania Del Santo, Barbara De Marco, Tiziana Di Salvo, Chris Done, Michal Dovčiak, Andrew C. Fabian, Maurizio Falanga, Angelo Francesco Gambino, Bruce Gendre, Victoria Grinberg, Alexander Heger, Jeroen Homan, Rosario Iaria, Jia Chen Jiang, Chi Chuan Jin, Elmar Koerding, Manu Linares, Zhu Liu, Thomas J. Maccarone, Julien Malzac, Antonios Manousakis, Frédéric Marin, Andrea Marinucci, Missagh Mehdipour, Mariano Méndez, Simone Migliari, Cole Miller, Giovanni Miniutti, Emanuele Nardini, Paul T. O’Brien, Julian P. Osborne, Pierre Olivier Petrucci, Andrea Possenti, Alessandro Riggio, Jerome Rodriguez, Andrea Sanna, Li Jing Shao, Malgosia Sobolewska, Eva Sramkova, Abigail L. Stevens, Holger Stiele, Giulia Stratta, Zdenek Stuchlik, Jiri Svoboda, Fabrizio Tamburini, Thomas M. Tauris, Francesco Tombesi, Gabriel Torok, Martin Urbanec, Frederic Vincent, Qing Wen Wu, Feng Yuan, Jean J.M. in’ t Zand, Andrzej A. Zdziarski, Xin Lin Zhou

Research output: Contribution to journal › Review article › peer-review

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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

Original language	English
Article number	29504
Journal	Science China: Physics, Mechanics and Astronomy
Volume	62
Issue number	2
DOIs	https://doi.org/10.1007/s11433-018-9297-0
Publication status	Published - 1 Feb 2019
Externally published	Yes

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http://adsabs.harvard.edu/abs/2019SCPMA..6229504D

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De Rosa, A., Uttley, P., Gou, L. J., Liu, Y., Bambi, C., Barret, D., Belloni, T., Berti, E., Bianchi, S., Caiazzo, I., Casella, P., Feroci, M., Ferrari, V., Gualtieri, L., Heyl, J., Ingram, A., Karas, V., Lu, F. J., Luo, B., ... Zhou, X. L. (2019). Accretion in strong field gravity with eXTP. Science China: Physics, Mechanics and Astronomy, 62(2), [29504]. https://doi.org/10.1007/s11433-018-9297-0

@article{38e730e7a8204e959d68f227c573e24b,

title = "Accretion in strong field gravity with eXTP",

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",

keywords = "X-ray, black holes physics, accretion",

author = "{De Rosa}, Alessandra and Phil Uttley and Gou, {Li Jun} and Yuan Liu and Cosimo Bambi and Didier Barret and Tomaso Belloni and Emanuele Berti and Stefano Bianchi and Ilaria Caiazzo and Piergiorgio Casella and Marco Feroci and Valeria Ferrari and Leonardo Gualtieri and Jeremy Heyl and Adam Ingram and Vladimir Karas and Lu, {Fang Jun} and Bin Luo and Giorgio Matt and Sara Motta and Joseph Neilsen and Paolo Pani and Andrea Santangelo and Shu, {Xin Wen} and Wang, {Jun Feng} and Wang, {Jian Min} and Xue, {Yong Quan} and Xu, {Yu Peng} and Yuan, {Wei Min} and Yuan, {Ye Fei} and Zhang, {Shuang Nan} and Shu Zhang and Ivan Agudo and Lorenzo Amati and Nils Andersson and Cristina Baglio and Pavel Bakala and Altan Baykal and Sudip Bhattacharyya and Ignazio Bombaci and Niccol{\'o} Bucciantini and Fiamma Capitanio and Riccardo Ciolfi and Cui, {Wei K.} and Filippo D{\textquoteright}Ammando and Thomas Dauser and {Del Santo}, Melania and {De Marco}, Barbara and {Di Salvo}, Tiziana and Chris Done and Michal Dov{\v c}iak and Fabian, {Andrew C.} and Maurizio Falanga and Gambino, {Angelo Francesco} and Bruce Gendre and Victoria Grinberg and Alexander Heger and Jeroen Homan and Rosario Iaria and Jiang, {Jia Chen} and Jin, {Chi Chuan} and Elmar Koerding and Manu Linares and Zhu Liu and Maccarone, {Thomas J.} and Julien Malzac and Antonios Manousakis and Fr{\'e}d{\'e}ric Marin and Andrea Marinucci and Missagh Mehdipour and Mariano M{\'e}ndez and Simone Migliari and Cole Miller and Giovanni Miniutti and Emanuele Nardini and O{\textquoteright}Brien, {Paul T.} and Osborne, {Julian P.} and Petrucci, {Pierre Olivier} and Andrea Possenti and Alessandro Riggio and Jerome Rodriguez and Andrea Sanna and Shao, {Li Jing} and Malgosia Sobolewska and Eva Sramkova and Stevens, {Abigail L.} and Holger Stiele and Giulia Stratta and Zdenek Stuchlik and Jiri Svoboda and Fabrizio Tamburini and Tauris, {Thomas M.} and Francesco Tombesi and Gabriel Torok and Martin Urbanec and Frederic Vincent and Wu, {Qing Wen} and Feng Yuan and {in{\textquoteright} t Zand}, {Jean J.M.} and Zdziarski, {Andrzej A.} and Zhou, {Xin Lin}",

year = "2019",

month = feb,

day = "1",

doi = "10.1007/s11433-018-9297-0",

language = "English",

volume = "62",

journal = "Science China: Physics, Mechanics and Astronomy",

issn = "1674-7348",

publisher = "Science Press",

number = "2",

}

De Rosa, A, Uttley, P, Gou, LJ, Liu, Y, Bambi, C, Barret, D, Belloni, T, Berti, E, Bianchi, S, Caiazzo, I, Casella, P, Feroci, M, Ferrari, V, Gualtieri, L, Heyl, J, Ingram, A, Karas, V, Lu, FJ, Luo, B, Matt, G, Motta, S, Neilsen, J, Pani, P, Santangelo, A, Shu, XW, Wang, JF, Wang, JM, Xue, YQ, Xu, YP, Yuan, WM, Yuan, YF, Zhang, SN, Zhang, S, Agudo, I, Amati, L, Andersson, N, Baglio, C, Bakala, P, Baykal, A, Bhattacharyya, S, Bombaci, I, Bucciantini, N, Capitanio, F, Ciolfi, R, Cui, WK, D’Ammando, F, Dauser, T, Del Santo, M, De Marco, B, Di Salvo, T, Done, C, Dovčiak, M, Fabian, AC, Falanga, M, Gambino, AF, Gendre, B, Grinberg, V, Heger, A, Homan, J, Iaria, R, Jiang, JC, Jin, CC, Koerding, E, Linares, M, Liu, Z, Maccarone, TJ, Malzac, J, Manousakis, A, Marin, F, Marinucci, A, Mehdipour, M, Méndez, M, Migliari, S, Miller, C, Miniutti, G, Nardini, E, O’Brien, PT, Osborne, JP, Petrucci, PO, Possenti, A, Riggio, A, Rodriguez, J, Sanna, A, Shao, LJ, Sobolewska, M, Sramkova, E, Stevens, AL, Stiele, H, Stratta, G, Stuchlik, Z, Svoboda, J, Tamburini, F, Tauris, TM, Tombesi, F, Torok, G, Urbanec, M, Vincent, F, Wu, QW, Yuan, F, in’ t Zand, JJM, Zdziarski, AA & Zhou, XL 2019, 'Accretion in strong field gravity with eXTP', Science China: Physics, Mechanics and Astronomy, vol. 62, no. 2, 29504. https://doi.org/10.1007/s11433-018-9297-0

TY - JOUR

T1 - Accretion in strong field gravity with eXTP

AU - De Rosa, Alessandra

AU - Uttley, Phil

AU - Gou, Li Jun

AU - Liu, Yuan

AU - Bambi, Cosimo

AU - Barret, Didier

AU - Belloni, Tomaso

AU - Berti, Emanuele

AU - Bianchi, Stefano

AU - Caiazzo, Ilaria

AU - Casella, Piergiorgio

AU - Feroci, Marco

AU - Ferrari, Valeria

AU - Gualtieri, Leonardo

AU - Heyl, Jeremy

AU - Ingram, Adam

AU - Karas, Vladimir

AU - Lu, Fang Jun

AU - Luo, Bin

AU - Matt, Giorgio

AU - Motta, Sara

AU - Neilsen, Joseph

AU - Pani, Paolo

AU - Santangelo, Andrea

AU - Shu, Xin Wen

AU - Wang, Jun Feng

AU - Wang, Jian Min

AU - Xue, Yong Quan

AU - Xu, Yu Peng

AU - Yuan, Wei Min

AU - Yuan, Ye Fei

AU - Zhang, Shuang Nan

AU - Zhang, Shu

AU - Agudo, Ivan

AU - Amati, Lorenzo

AU - Andersson, Nils

AU - Baglio, Cristina

AU - Bakala, Pavel

AU - Baykal, Altan

AU - Bhattacharyya, Sudip

AU - Bombaci, Ignazio

AU - Bucciantini, Niccoló

AU - Capitanio, Fiamma

AU - Ciolfi, Riccardo

AU - Cui, Wei K.

AU - D’Ammando, Filippo

AU - Dauser, Thomas

AU - Del Santo, Melania

AU - De Marco, Barbara

AU - Di Salvo, Tiziana

AU - Done, Chris

AU - Dovčiak, Michal

AU - Fabian, Andrew C.

AU - Falanga, Maurizio

AU - Gambino, Angelo Francesco

AU - Gendre, Bruce

AU - Grinberg, Victoria

AU - Heger, Alexander

AU - Homan, Jeroen

AU - Iaria, Rosario

AU - Jiang, Jia Chen

AU - Jin, Chi Chuan

AU - Koerding, Elmar

AU - Linares, Manu

AU - Liu, Zhu

AU - Maccarone, Thomas J.

AU - Malzac, Julien

AU - Manousakis, Antonios

AU - Marin, Frédéric

AU - Marinucci, Andrea

AU - Mehdipour, Missagh

AU - Méndez, Mariano

AU - Migliari, Simone

AU - Miller, Cole

AU - Miniutti, Giovanni

AU - Nardini, Emanuele

AU - O’Brien, Paul T.

AU - Osborne, Julian P.

AU - Petrucci, Pierre Olivier

AU - Possenti, Andrea

AU - Riggio, Alessandro

AU - Rodriguez, Jerome

AU - Sanna, Andrea

AU - Shao, Li Jing

AU - Sobolewska, Malgosia

AU - Sramkova, Eva

AU - Stevens, Abigail L.

AU - Stiele, Holger

AU - Stratta, Giulia

AU - Stuchlik, Zdenek

AU - Svoboda, Jiri

AU - Tamburini, Fabrizio

AU - Tauris, Thomas M.

AU - Tombesi, Francesco

AU - Torok, Gabriel

AU - Urbanec, Martin

AU - Vincent, Frederic

AU - Wu, Qing Wen

AU - Yuan, Feng

AU - in’ t Zand, Jean J.M.

AU - Zdziarski, Andrzej A.

AU - Zhou, Xin Lin

PY - 2019/2/1

Y1 - 2019/2/1

N2 - 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

AB - 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

KW - X-ray

KW - black holes physics

KW - accretion

UR - http://www.scopus.com/inward/record.url?scp=85054141547&partnerID=8YFLogxK

U2 - 10.1007/s11433-018-9297-0

DO - 10.1007/s11433-018-9297-0

M3 - Review article

SN - 1674-7348

VL - 62

JO - Science China: Physics, Mechanics and Astronomy

JF - Science China: Physics, Mechanics and Astronomy

IS - 2

M1 - 29504

ER -

Accretion in strong field gravity with eXTP

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