Inner disc obscuration in GRS 1915+105 based on relativistic slim disc model
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F13%3A00422973" target="_blank" >RIV/67985815:_____/13:00422973 - isvavai.cz</a>
Result on the web
<a href="http://dx.doi.org/10.1093/mnras/stt1467" target="_blank" >http://dx.doi.org/10.1093/mnras/stt1467</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1093/mnras/stt1467" target="_blank" >10.1093/mnras/stt1467</a>
Alternative languages
Result language
angličtina
Original language name
Inner disc obscuration in GRS 1915+105 based on relativistic slim disc model
Original language description
We study the observational signatures of the relativistic slim disc of 10 M-circle dot black hole, in a wide range of mass accretion rate, (m) over dot, dimensionless spin parameter, a(*), and viewing angle, i.
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
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace
Others
Publication year
2013
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Name of the periodical
Monthly Notices of the Royal Astronomical Society
ISSN
0035-8711
e-ISSN
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Volume of the periodical
436
Issue of the periodical within the volume
1
Country of publishing house
GB - UNITED KINGDOM
Number of pages
11
Pages from-to
71-81
UT code for WoS article
000326435100028
EID of the result in the Scopus database
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