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.
Sign-in/Register to access full text options 
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callMore From: International Journal of Modern Physics: Conference Series
Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
