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Disk-Jet Connection in Black Holes

  • Arghajit Jana
Conference paper
Part of the Astrophysics and Space Science Proceedings book series (ASSSP, volume 53)

Abstract

It is well established that the accretion disk and jet are coupled. Jet and accretion disk arise self-consistently from any transonic flow solution and clearly from its generalized version, the two-component advective flow (TCAF) solution. Observationally, strong signatures of disk-jet connections are seen for many black hole binaries. The nature and evolution of jets depend on accretion flows. Correlation between X-ray and radio fluxes is also seen, which indicates a coupling between accretion disk and jet. In this review, we discuss developments of theoretical models to describe the origin of the jets or outflows and the nature of the disk-jet coupling on the basis of the transonic flows around black holes. Then we discuss the observational evidences of the disk-jet connections.

Notes

Acknowledgements

I would like to thank Prof. Sandip K. Chakrabarti and Dr. Dipak Debnath for guiding me in my academic career. I would also like to thank ICSP, ISRO, DST and CSIR for their financial assistance to me.

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Copyright information

© Springer International Publishing AG, part of Springer Nature 2018

Authors and Affiliations

  • Arghajit Jana
    • 1
  1. 1.Indian Centre for Space PhysicsKolkataIndia

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