We obtained global transonic solutions representing optically thin advection-dominated accretion flow by solving the full set of differential equations describing such systems. We found that far from the sonic point self-similar solutions are an excellent approximation of the global flow structure if the accretion rate is well below the maximum value above which no optically thin solutions exist. © 1997. The American Astronomical Society. All rights reserved.
CITATION STYLE
Chen, X., Abramowicz, M. A., & Lasota, J. (1997). Advection‐dominated Accretion: Global Transonic Solutions. The Astrophysical Journal, 476(1), 61–69. https://doi.org/10.1086/303592
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