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A magnetized torus for modeling Sagittarius A* millimeter images and spectra

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F47813059%3A19240%2F15%3A%230005468" target="_blank" >RIV/47813059:19240/15:#0005468 - isvavai.cz</a>

  • Result on the web

    <a href="http://www.aanda.org/articles/aa/abs/2015/02/aa24306-14/aa24306-14.html" target="_blank" >http://www.aanda.org/articles/aa/abs/2015/02/aa24306-14/aa24306-14.html</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1051/0004-6361/201424306" target="_blank" >10.1051/0004-6361/201424306</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    A magnetized torus for modeling Sagittarius A* millimeter images and spectra

  • Original language description

    The supermassive black hole, Sagittarius (Sgr) A*, in the centre of our Galaxy has the largest angular size in the sky among all astrophysical black holes. Its shadow, assuming no rotation, spans similar to 50 mu as. Resolving such dimensions has long been out of reach for astronomical instruments until a new generation of interferometers being operational during this decade. Of particular interest is the Event Horizon Telescope (EHT) with resolution similar to 20 mu as in the millimeter- wavelength range 0.87 mm - 1.3 mm. We investigate the ability of the fully general relativistic Komissarov (2006, MNRAS, 368, 993) analytical magnetized torus model to account for observable constraints at Sgr A* in the centimeter and millimeter domains. The impact ofthe magnetic field geometry on the observables is also studied. We show that the torus model is capable of reproducing spectral constraints in the millimeter domain, and in particular in the observable domain of the EHT. However, the tor

  • Czech name

  • Czech description

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

Result continuities

  • Project

    <a href="/en/project/EE2.3.20.0071" target="_blank" >EE2.3.20.0071: Supporting Integration with the International Theoretical and Observational Research Network in Relativistic Astrophysics of Compact Objects</a><br>

  • Continuities

    P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)<br>I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Others

  • Publication year

    2015

  • Confidentiality

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

Data specific for result type

  • Name of the periodical

    Astronomy & Astrophysics

  • ISSN

    0004-6361

  • e-ISSN

  • Volume of the periodical

    574

  • Issue of the periodical within the volume

    February

  • Country of publishing house

    FR - FRANCE

  • Number of pages

    9

  • Pages from-to

    "A48-1"-"A48-9"

  • UT code for WoS article

    000349467000048

  • EID of the result in the Scopus database

    2-s2.0-84921470087