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Accretion in strong field gravity with eXTP

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dc.contributor.authorDe Rosa, A.
dc.contributor.authorUttley, P.
dc.contributor.authorGou, L.
dc.contributor.authorLiu, Y.
dc.contributor.authorBambi, C.
dc.contributor.authorBarret, Didier
dc.contributor.authorBelloni, T.
dc.contributor.authorBerti, E.
dc.contributor.authorBianchi, S.
dc.contributor.authorCaiazzo, I.
dc.contributor.authorCasella, P.
dc.contributor.authorCui, W. K.
dc.contributor.authorD´Ammando, F.
dc.contributor.authorDauser, T.
dc.contributor.authorDel Santo, M.
dc.contributor.authorDe Marco, B.
dc.contributor.authorDi Salvo, T.
dc.contributor.authorDone, C.
dc.contributor.authorDovciak, M.
dc.contributor.authorFabian, A. C.
dc.contributor.authorFalanga, M.
dc.contributor.authorGambino, A. F.
dc.contributor.authorGendre, B.
dc.contributor.authorGrinberg, V.
dc.contributor.authorHeger, A.
dc.contributor.authorHoman, J.
dc.contributor.authorIaria, R.
dc.contributor.authorJiang, J.
dc.contributor.authorJin, C. C.
dc.contributor.authorKoerding, E.
dc.contributor.authorLinares, M.
dc.contributor.authorLiu, Z.
dc.contributor.authorMaccarone, Thomas J.
dc.contributor.authorMalzac, J.
dc.contributor.authorManousakis, A.
dc.contributor.authorMarin, F.
dc.contributor.authorMarinucci, A.
dc.contributor.authorMehdipour, M.
dc.contributor.authorMéndez, M.
dc.contributor.authorMigliari, S.
dc.contributor.authorMiller, C.
dc.contributor.authorMiniutti, G.
dc.contributor.authorNardini, E.
dc.contributor.authorO´Brien, P. T.
dc.contributor.authorOsborne, Julian P.
dc.contributor.authorPetrucci, P. O.
dc.contributor.authorPossenti, A.
dc.contributor.authorRiggio, A.
dc.contributor.authorRodríguez, J.
dc.contributor.authorSanna, A.
dc.contributor.authorShao, L. J.
dc.contributor.authorSobolewska, M.
dc.contributor.authorSramkova, E.
dc.contributor.authorStevens, A. L.
dc.contributor.authorStiele, H.
dc.contributor.authorStratta, G.
dc.contributor.authorStuchlik, Z.
dc.contributor.authorSvoboda, J.
dc.contributor.authorTamburini, F.
dc.contributor.authorTauris, T. M.
dc.contributor.authorTombesi, F.
dc.contributor.authorTorok, G.
dc.contributor.authorUrbanec, M.
dc.contributor.authorVicent, F.
dc.contributor.authorWu, Q. W.
dc.contributor.authorYuan, F.
dc.contributor.authorZand, J. J. M.
dc.contributor.authorZdziarski, A. A.
dc.contributor.authorZhou, X.
dc.contributor.authorFeroci, M.
dc.contributor.authorFerrari, V.
dc.contributor.authorGualtieri, L.
dc.contributor.authorHeyl, J.
dc.contributor.authorIngram, A.
dc.contributor.authorKaras, V.
dc.contributor.authorLu, F. J.
dc.contributor.authorLuo, B.
dc.contributor.authorMatt, G.
dc.contributor.authorMotta, S. E.
dc.contributor.authorNeilsen, J.
dc.contributor.authorPani, P.
dc.contributor.authorSantangelo, A.
dc.contributor.authorShu, X. W.
dc.contributor.authorWang, J. F.
dc.contributor.authorWang, J. M.
dc.contributor.authorXue, Y. Q.
dc.contributor.authorXu, Y. P.
dc.contributor.authorYuan, W. M.
dc.contributor.authorYuan, Y. F.
dc.contributor.authorZhang, S. N.
dc.contributor.authorZhang, S.
dc.contributor.authorAgudo, I.
dc.contributor.authorAmati, L.
dc.contributor.authorAndersson, N. A.
dc.contributor.authorBaglio, C.
dc.contributor.authorBakala, P.
dc.contributor.authorBaykal, A.
dc.contributor.authorBhattacharyya, S.
dc.contributor.authorBombaci, I.
dc.contributor.authorBucciantini, N.
dc.contributor.authorCapitanio, F.
dc.contributor.authorCiolfi, R.
dc.contributor.funderIstituto Nazionale di Astrofisica (INAF)
dc.contributor.funderChinese Academy of Sciences (CAS)
dc.contributor.funderNational Science Centre, Poland (NCN)
dc.date.accessioned2021-09-27T10:48:41Z
dc.date.available2021-09-27T10:48:41Z
dc.date.issued2018-12-07
dc.description.abstractIn 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-spinmeasurementses
dc.description.sponsorshipThe Italian collaboration acknowledged financial contribution from the agreement ASI-INAF n.2017-14-H.O. The Chinese team acknowledged the support of the Chinese Academy of Sciences through the Strategic Priority Research Program of the Chinese Academy of Sciences (Grant No. XDA15020100). A. Zdziarski acknowledges the Polish National Science Centre (Grant No. 2013/10/M/ST9/00729).es
dc.identifier.citationScience China Physics, Mechanics & Astronomy 62(2): A029504(2019)es
dc.identifier.doi10.1007/s11433-018-9297-0
dc.identifier.e-issn1869-1927
dc.identifier.issn1674-7348
dc.identifier.otherhttps://link.springer.com/article/10.1007%2Fs11433-018-9297-0
dc.identifier.urihttp://hdl.handle.net/20.500.12666/471
dc.language.isoenges
dc.publisherSpringer Linkes
dc.rights.accessRightsinfo:eu-repo/semantics/restrictedAccess
dc.rights.licenseCopyright © 2018, Science China Press and Springer-Verlag GmbH Germany, part of Springer Nature
dc.subjectX rayes
dc.subjectBlack holes physicses
dc.subjectAccretiones
dc.titleAccretion in strong field gravity with eXTPes
dc.typeinfo:eu-repo/semantics/articlees
dc.type.coarhttp://purl.org/coar/resource_type/c_6501
dc.type.hasVersioninfo:eu-repo/semantics/publishedVersion
dspace.entity.typePublication

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