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  • We discuss the general relativity effects acting on the radiation signal from the inner accretion flow. We consider the radiation flux and polarization properties originating from a blob of gas near a rotating black hole. The predicted observed polarization at infinity is changed from its local value due to strong gravity and fast orbital motion. Different processes can produce the observed pattern: in the context of Sgr A* flares, the synchrotron mechanism and the inverse Compton up-scattering appear to be the most likely mechanisms.
  • We discuss the general relativity effects acting on the radiation signal from the inner accretion flow. We consider the radiation flux and polarization properties originating from a blob of gas near a rotating black hole. The predicted observed polarization at infinity is changed from its local value due to strong gravity and fast orbital motion. Different processes can produce the observed pattern: in the context of Sgr A* flares, the synchrotron mechanism and the inverse Compton up-scattering appear to be the most likely mechanisms. (en)
Title
  • Revealing the general relativity effects in accretion events near a supermassive black hole
  • Revealing the general relativity effects in accretion events near a supermassive black hole (en)
skos:prefLabel
  • Revealing the general relativity effects in accretion events near a supermassive black hole
  • Revealing the general relativity effects in accretion events near a supermassive black hole (en)
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  • RIV/67985815:_____/11:00359757!RIV12-AV0-67985815
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  • P(GA205/07/0052), Z(AV0Z10030501)
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  • 226898
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  • RIV/67985815:_____/11:00359757
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  • galactic centre (en)
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  • [D0EF0D2E5BE4]
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  • Shanghai
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  • The Galactic Center: A Window to the Nuclear Environment of Disk Galaxies
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  • Dovčiak, Michal
  • Eckart, A.
  • Karas, Vladimír
  • Zamaninasab, M.
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http://linked.open...ain/vavai/riv/wos
  • 000291890200067
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number of pages
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  • Astronomical Society of the Pacific
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  • 978-1-58381-758-2
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