Role of the emission angular directionality in the spin determination of 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%3A00345822" target="_blank" >RIV/67985815:_____/10:00345822 - isvavai.cz</a>
Result on the web
<a href="http://dx.doi.org/10.1063/1.3475328" target="_blank" >http://dx.doi.org/10.1063/1.3475328</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1063/1.3475328" target="_blank" >10.1063/1.3475328</a>
Alternative languages
Result language
angličtina
Original language name
Role of the emission angular directionality in the spin determination of accreting black holes
Original language description
We discuss the method to determine black hole spin with relativistic models of iron line. We study how sensitive the spin measurements are to the assumption about emission directionality of the reflected radiation from the disc.
Czech name
—
Czech description
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Classification
Type
D - Article in proceedings
CEP classification
BN - Astronomy and celestial mechanics, astrophysics
OECD FORD branch
—
Result continuities
Project
—
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 astronomy 2009: Present status, multi-wavelength approach and future perspectives
ISBN
978-0-7354-0795-4
ISSN
0094-243X
e-ISSN
—
Number of pages
2
Pages from-to
515-516
Publisher name
American Institute of Physics
Place of publication
Melville
Event location
Bologna
Event date
Sep 7, 2009
Type of event by nationality
WRD - Celosvětová akce
UT code for WoS article
000284017700178