On the driver of relativistic effect strength in Seyfert galaxies
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F11%3A00370926" target="_blank" >RIV/67985815:_____/11:00370926 - isvavai.cz</a>
Result on the web
<a href="http://dx.doi.org/10.1051/0004-6361/201016245" target="_blank" >http://dx.doi.org/10.1051/0004-6361/201016245</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1051/0004-6361/201016245" target="_blank" >10.1051/0004-6361/201016245</a>
Alternative languages
Result language
angličtina
Original language name
On the driver of relativistic effect strength in Seyfert galaxies
Original language description
Spectroscopy of X-ray emission lines emitted from accretion discs around super-massive black holes provides in principle observational constraints on the black hole spin. Previous studies have suggested that relativistically broadened line profiles are fairly common in nearby unobscured Seyfert galaxies. Their strength spans a range of almost two orders of magnitude. We attempt to determine the ultimate physical driver of the strength of this relativistic reprocessing feature.
Czech name
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Czech description
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Classification
Type
J<sub>x</sub> - Unclassified - Peer-reviewed scientific article (Jimp, Jsc and Jost)
CEP classification
BN - Astronomy and celestial mechanics, astrophysics
OECD FORD branch
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Result continuities
Project
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Continuities
Z - Vyzkumny zamer (s odkazem do CEZ)
Others
Publication year
2011
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Name of the periodical
Astronomy and Astrophysics
ISSN
0004-6361
e-ISSN
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Volume of the periodical
531
Issue of the periodical within the volume
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Country of publishing house
FR - FRANCE
Number of pages
13
Pages from-to
"A131/1"-"A131/13"
UT code for WoS article
000293017700055
EID of the result in the Scopus database
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