Spectral Signature of Mass Outflow in the Two Component Advective Flow Paradigm

@article{Mondal2021SpectralSO,
  title={Spectral Signature of Mass Outflow in the Two Component Advective Flow Paradigm},
  author={Santanu Mondal and Sandip Kumar Chakrabarti},
  journal={The Astrophysical Journal},
  year={2021},
  volume={920}
}
  • Santanu Mondal, S. Chakrabarti
  • Published 2021
  • Physics
  • The Astrophysical Journal
Outflows are common in many astrophysical systems. In the Two Component Advective Flow (TCAF) paradigm, which is essentially a generalized Bondi flow including rotation, viscosity, and cooling effects, the outflow originates in the hot, puffed up, post-shock region at the inner edge of the accretion disk. We consider this region to be the base of the jet carrying away matter with a high velocity. In this paper, we study the spectral properties of black holes using TCAF that includes also a jet… Expand

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