Accretion in strong field gravity with eXTP

0517416 - ASÚ 2020 RIV CN eng J - Článek v odborném periodiku
de Rosa, A. - Uttley, P. - Gou, L. - Liu, Y. - Bambi, C. - Barret, D. - Belloni, T. - Karas, Vladimír - Dovčiak, Michal - Svoboda, Jiří … celkem 102 autorů
Accretion in strong field gravity with eXTP.
Science China Physics, Mechanics & Astronomy. Roč. 62, č. 2 (2019), č. článku 029504. ISSN 1674-7348. E-ISSN 1869-1927
Institucionální podpora: RVO:67985815
Klíčová slova: X-ray * black holes physics * accretion
Obor OECD: Astronomy (including astrophysics,space science)
Impakt faktor: 4.226, rok: 2019
Způsob publikování: Omezený přístup
https://doi.org/10.1007/s11433-018-9297-0

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.
Trvalý link: http://hdl.handle.net/11104/0302728