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Spectra of puffy accretion discs: the kynbb fit

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F23%3A00575374" target="_blank" >RIV/67985815:_____/23:00575374 - isvavai.cz</a>

  • Alternative codes found

    RIV/47813059:19630/23:A0000256 RIV/00216208:11320/23:10468725

  • Result on the web

    <a href="https://doi.org/10.1002/asna.20230023" target="_blank" >https://doi.org/10.1002/asna.20230023</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1002/asna.20230023" target="_blank" >10.1002/asna.20230023</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Spectra of puffy accretion discs: the kynbb fit

  • Original language description

    Puffy disc is a numerical model, expected to capture the properties of the accretion flow in X‑ray black hole (BH) binaries in the luminous, mildly sub‑Eddington state. We fit the kerrbb and kynbb spectral models in XSPEC to synthetic spectra of puffy accretion discs, obtained in general relativistic radiative magnetohydrodynamic simulations, to see if they correctly recover the BH spin and mass accretion rate assumed in the numerical simulation. We conclude that neither of the two models is capable of correctly recovering the puffy disc parameters, which highlights a necessity to develop new, more accurate spectral models for the luminous regime of accretion in X‑ray BH binaries. We propose that such spectral models should be based on the results of numerical simulations of accretion.n

  • Czech name

  • Czech description

Classification

  • Type

    J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database

  • CEP classification

  • OECD FORD branch

    10308 - Astronomy (including astrophysics,space science)

Result continuities

  • Project

    Result was created during the realization of more than one project. More information in the Projects tab.

  • Continuities

    I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Others

  • Publication year

    2023

  • Confidentiality

    S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Data specific for result type

  • Name of the periodical

    Astronomische Nachrichten

  • ISSN

    0004-6337

  • e-ISSN

    1521-3994

  • Volume of the periodical

    344

  • Issue of the periodical within the volume

    4

  • Country of publishing house

    US - UNITED STATES

  • Number of pages

    6

  • Pages from-to

    e20230023

  • UT code for WoS article

    000924154300001

  • EID of the result in the Scopus database

    2-s2.0-85147363681