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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

  • Czech description

Classification

  • Type

    D - Article in proceedings

  • CEP classification

  • 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

  • ISSN

    1405-2059

  • e-ISSN

  • 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