Accretion in strong field gravity with eXTP

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F19%3A00517416" target="_blank" >RIV/67985815:_____/19:00517416 - isvavai.cz</a>
Alternative codes found
RIV/47813059:19240/19:A0000532
Result on the web
<a href="https://doi.org/10.1007/s11433-018-9297-0" target="_blank" >https://doi.org/10.1007/s11433-018-9297-0</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1007/s11433-018-9297-0" target="_blank" >10.1007/s11433-018-9297-0</a>

Result language
angličtina
Original language name
Accretion in strong field gravity with eXTP
Original language description
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.
Czech name
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Czech description
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Type
J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database
CEP classification
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OECD FORD branch
10308 - Astronomy (including astrophysics,space science)

Project
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Continuities
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Publication year
2019
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

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