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- W3100208862 abstract "I review radiatively inefficient accretion flow models for the ≈2.6 × 106 M⊙ black hole (BH) in the Galactic Center. I argue for a ‘concordance model’ of Sgr A*: both theory and observations suggest that hot ambient gas around the BH is accreted at a rate ∼10–8 M⊙ yr–1 much less than the canonical Bondi rate. I interpret Chandra observations of Sgr A* in the context of such a model: (1) the extended ‘quiescent’ X-ray emission is due to thermal bremsstrahlung from gas in the vicinity of the Bondi accretion radius, and (2) the ∼104 second long X-ray flares are due to synchrotron or Inverse-Compton emission by non-thermal electrons accelerated in the inner ∼10 Schwarzschild radii of the accretion flow." @default.
- W3100208862 created "2020-11-23" @default.
- W3100208862 creator A5000130235 @default.
- W3100208862 date "2003-09-01" @default.
- W3100208862 modified "2023-10-16" @default.
- W3100208862 title "Radiatively Inefficient Accretion Flow Models of Sgr A*" @default.
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- W3100208862 doi "https://doi.org/10.1002/asna.200385043" @default.
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