Future polarimetry of orbiting blobs in accretion discs

@proceedings{53631,
   author = {Karas, Vladimír and Zajaček, Michal and Eckart, Andreas},
   booktitle = {RAGtime 23: 6-10 September, 2021 - Workshop on Black Holes and Neutron Stars},
   language = {eng},
   title = {Future polarimetry of orbiting blobs in accretion discs},
   url = {https://indico.slu.cz/event/8/contributions/110/},
   year = {2021}
}

TY  - CONF
ID  - 53631
AU  - Karas, Vladimír - Zajaček, Michal - Eckart, Andreas
PY  - 2021
TI  - Future polarimetry of orbiting blobs in accretion discs
UR  - https://indico.slu.cz/event/8/contributions/110/
N2  - Energy shifts of radiation from accreting black holes may be caused by the fast orbital motion and the gravitational redshift near the event horizon. Individual clumps of matter experience the effects of general relativity as they gradually fall into a deep potential well. An episodic supply of material is maintained by tidal disruption events and the emerging radiation is modulated in the X-ray domain and in longer wavelengths. Changes of polarization properties of the observed signal exhibit a specific dependence on energy and phase.
ER  - 

KARAS, Vladimír, Michal ZAJAČEK a Andreas ECKART. Future polarimetry of orbiting blobs in accretion discs. In \textit{RAGtime 23: 6-10 September, 2021 - Workshop on Black Holes and Neutron Stars}. 2021.