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- W2012419755 abstract "A recently discovered transient X-ray source, IGR J17177-3656, has received many observations, including a quasi-simultaneous multi-waveband observations. The source is modeled with the coupled accretion-jet model around a black hole. It is found that the multi-waveband spectrum can be successfully modeled with the luminous hot accretion flow (LHAF) rather than advection dominated accretion flow (ADAF). The modeled luminosity is about 5% of the Eddington luminosity, and the source may be as far as 25 kpc. Our detailed modeling result confirms the point that LHAF can explain steep radio-X-ray correlation." @default.
- W2012419755 created "2016-06-24" @default.
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- W2012419755 date "2013-01-01" @default.
- W2012419755 modified "2023-10-16" @default.
- W2012419755 title "LUMINOUS HOT ACCRETION FLOW AND THE MODELING OF THE MULTI-BAND SPECTRUM OF IGR J17177-3656" @default.
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- W2012419755 doi "https://doi.org/10.1142/s201019451301101x" @default.
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