X-ray polarization fluctuations induced by cloud eclipses in active galactic nuclei
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F15%3A00438422" target="_blank" >RIV/67985815:_____/15:00438422 - isvavai.cz</a>
Result on the web
<a href="http://dx.doi.org/10.1051/0004-6361/201424862" target="_blank" >http://dx.doi.org/10.1051/0004-6361/201424862</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1051/0004-6361/201424862" target="_blank" >10.1051/0004-6361/201424862</a>
Alternative languages
Result language
angličtina
Original language name
X-ray polarization fluctuations induced by cloud eclipses in active galactic nuclei
Original language description
We find that X-ray polarimetry is particularly adapted to probing X-ray eclipses due to Compton-thin and Compton-thick gas clouds. Polarization measurements would distinguish between intrinsic intensity fluctuations and external eclipsing events, constrain the geometry of the covering medium, and test the hypothesis of non-uniformly emitting disks predicted by general relativity.
Czech name
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Czech description
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Classification
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)
Result continuities
Project
<a href="/en/project/LD12010" target="_blank" >LD12010: X-ray polarization from accretion discs</a><br>
Continuities
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace
Others
Publication year
2015
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Name of the periodical
Astronomy & Astrophysics
ISSN
1432-0746
e-ISSN
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Volume of the periodical
573
Issue of the periodical within the volume
January
Country of publishing house
US - UNITED STATES
Number of pages
8
Pages from-to
"A60/1"-"A60/8"
UT code for WoS article
000346901300086
EID of the result in the Scopus database
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