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Accretion in strong field gravity with eXTP
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SYSNO ASEP 0517416 Document Type J - Journal Article R&D Document Type Journal Article Subsidiary J Článek ve WOS Title Accretion in strong field gravity with eXTP Author(s) de Rosa, A. (IT)
Uttley, P. (NL)
Gou, L. (CN)
Liu, Y. (CN)
Bambi, C. (CN)
Barret, D. (FR)
Belloni, T. (IT)
Karas, Vladimír (ASU-R) RID, ORCID
Dovčiak, Michal (ASU-R) RID, ORCID
Svoboda, Jiří (ASU-R) RID, ORCIDNumber of authors 102 Article number 029504 Source Title Science China Physics, Mechanics & Astronomy. - : Zhongguo Kexue Zazhishe - ISSN 1674-7348
Roč. 62, č. 2 (2019)Number of pages 29 s. Publication form Online - E Language eng - English Country CN - China Keywords X-ray ; black holes physics ; accretion Subject RIV BN - Astronomy, Celestial Mechanics, Astrophysics OECD category Astronomy (including astrophysics,space science) Method of publishing Limited access Institutional support ASU-R - RVO:67985815 UT WOS 000459907400001 EID SCOPUS 85054141547 DOI 10.1007/s11433-018-9297-0 Annotation 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 out flows which are driven by the accretion process. Workplace Astronomical Institute Contact Radka Svašková, bibl@asu.cas.cz, Tel.: 323 620 326 Year of Publishing 2020 Electronic address https://doi.org/10.1007/s11433-018-9297-0
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