Matches in SemOpenAlex for { <https://semopenalex.org/work/W3088573456> ?p ?o ?g. }
- W3088573456 endingPage "154" @default.
- W3088573456 startingPage "154" @default.
- W3088573456 abstract "We review the physical origins for possible visible images of the supermassive black hole M87* in the galaxy M87 and SgrA* in the Milky Way Galaxy. The classical dark black hole shadow of the maximal size is visible in the case of luminous background behind the black hole at the distance exceeding the so-called photon spheres. The notably smaller dark shadow (dark silhouette) of the black hole event horizon is visible if the black hole is highlighted by the inner parts of the luminous accreting matter inside the photon spheres. The first image of the supermassive black hole M87*, obtained by the Event Horizon Telescope collaboration, shows the lensed dark image of the southern hemisphere of the black hole event horizon globe, highlighted by accreting matter, while the classical black hole shadow is invisible at all. A size of the dark spot on the Event Horizon Telescope (EHT) image agrees with a corresponding size of the dark event horizon silhouette in a thin accretion disk model in the case of either the high or moderate value of the black hole spin, a≳0.75." @default.
- W3088573456 created "2020-10-01" @default.
- W3088573456 creator A5061097449 @default.
- W3088573456 creator A5076618183 @default.
- W3088573456 date "2020-09-21" @default.
- W3088573456 modified "2023-10-01" @default.
- W3088573456 title "Visible Shapes of Black Holes M87* and SgrA*" @default.
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