Polarization of thermal emission from accreting black holes
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F10%3A00345563" target="_blank" >RIV/67985815:_____/10:00345563 - 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
Polarization of thermal emission from accreting black holes
Original language description
Multicolour black-body emission from the accretion disc around the black hole can be polarized on its way through the atmosphere above the accretion disc. We model this effect by assuming Kerr metric.
Czech name
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Czech description
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Classification
Type
D - Article in proceedings
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
2010
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Article name in the collection
X-ray polarimetry: A new window in astrophysics
ISBN
978-0-521-19184-5
ISSN
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e-ISSN
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Number of pages
5
Pages from-to
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Publisher name
Cambridge University Press
Place of publication
Cambridge
Event location
Rome
Event date
Apr 27, 2009
Type of event by nationality
WRD - Celosvětová akce
UT code for WoS article
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