Understanding the iron K alpha line emissivity profile with GR radiative transfer code
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F20%3A00539460" target="_blank" >RIV/67985815:_____/20:00539460 - isvavai.cz</a>
Result on the web
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DOI - Digital Object Identifier
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Alternative languages
Result language
angličtina
Original language name
Understanding the iron K alpha line emissivity profile with GR radiative transfer code
Original language description
In this work, we present calculations of the illumination and the iron K alpha emissivity profiles performed with the GR radiative transfer code Monk that employs the Monte Carlo method. In most previous studies the distinction between the illumination and emissivity profiles was not clearly made. For AGN discs, the emissivity profile has a similar shape with the illumination profile, but in the inner most region the former is steeper than the latter, where as for accretion discs in black hole X-ray binaries, the distinction between the two profiles is more dramatic. We find out that the different behavior between AGN and black hole X-ray binary discs is due to the different energy spectra of the illuminating radiation. This suggests that the emissivity profile of the iron Kαline cannot be determined by black hole spin and corona geometry alone and the energy spectrum of the illuminating radiation has to be taken into account. We also study the dependence of the emissivity profile on the geometry of the corona.
Czech name
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Czech description
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Classification
Type
D - Article in proceedings
CEP classification
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OECD FORD branch
10308 - Astronomy (including astrophysics,space science)
Result continuities
Project
<a href="/en/project/GA17-02430S" target="_blank" >GA17-02430S: Geometrical properties of the accretion disc corona in Active Galactic Nuclei</a><br>
Continuities
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace
Others
Publication year
2020
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Article name in the collection
Proceedings of RAGtime 20/22: Workshops on black holes and neutron stars
ISBN
978-80-7510-433-5
ISSN
2336-5676
e-ISSN
2336-5676
Number of pages
14
Pages from-to
383-396
Publisher name
Silesian University
Place of publication
Opava
Event location
Opava
Event date
Oct 15, 2018
Type of event by nationality
WRD - Celosvětová akce
UT code for WoS article
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