On The Search of the “Elusive” Intermediate Mass Black-Holes
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F19%3A00517318" target="_blank" >RIV/67985815:_____/19:00517318 - isvavai.cz</a>
Result on the web
<a href="http://dx.doi.org/10.22201/ia.14052059p.2019.51.16" target="_blank" >http://dx.doi.org/10.22201/ia.14052059p.2019.51.16</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.22201/ia.14052059p.2019.51.16" target="_blank" >10.22201/ia.14052059p.2019.51.16</a>
Alternative languages
Result language
angličtina
Original language name
On The Search of the “Elusive” Intermediate Mass Black-Holes
Original language description
Ultra-Luminous X-ray sources (ULXs) are accreting black holes for which their X-ray properties have been seen to be different to the case of stellar-mass black hole binaries. For most of the cases their intrinsic energy spectra are well described by a cold accretion disc (thermal) plus a curved high-energy emission components. The mass of the black hole (BH) derived from the thermal disc component is usually in the range of 100-105 solar masses, which have led to the idea that this can represent strong evidence of the Intermediate Mass Black Holes (IMBH), proposed to exist by theoretical studies but with no firm detection (as a class) so far. Recent theoretical and observational developments are leading towards the idea that these sources are instead compact objects accreting at an unusual super-Eddington regime instead. On the other hand, gravitational waves have been seen to be a useful tool for finding (some of these) IMBHs. We give a brief overview about the recent advent of the discovery of gravitational waves and their relationship with these so far elusive IMBHs.
Czech name
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Czech description
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Classification
Type
D - Article in proceedings
CEP classification
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OECD FORD branch
10308 - Astronomy (including astrophysics,space science)
Result continuities
Project
<a href="/en/project/GA18-00533S" target="_blank" >GA18-00533S: Reverberation from Black Hole accretion discs</a><br>
Continuities
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace
Others
Publication year
2019
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Article name in the collection
Workshop on Robotic Autonomous Observatories /5./
ISBN
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ISSN
1405-2059
e-ISSN
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Number of pages
9
Pages from-to
96-104
Publisher name
Universidad Nacional Autonoma de Mexico
Place of publication
Mexico City
Event location
Mazagon
Event date
Oct 16, 2017
Type of event by nationality
WRD - Celosvětová akce
UT code for WoS article
000480824300015