Probing the Physics of Active Galaxies Using Multi-wavelength Data

APA

Shastri, P. (2014). Probing the Physics of Active Galaxies Using Multi-wavelength Data. Perimeter Institute for Theoretical Physics. https://pirsa.org/14080000

MLA

Shastri, Prajval. Probing the Physics of Active Galaxies Using Multi-wavelength Data. Perimeter Institute for Theoretical Physics, Aug. 05, 2014, https://pirsa.org/14080000

BibTex

          @misc{ scivideos_PIRSA:14080000,
            doi = {10.48660/14080000},
            url = {https://pirsa.org/14080000},
            author = {Shastri, Prajval},
            keywords = {Cosmology},
            language = {en},
            title = {Probing the Physics of Active Galaxies Using Multi-wavelength Data},
            publisher = {Perimeter Institute for Theoretical Physics},
            year = {2014},
            month = {aug},
            note = {PIRSA:14080000 see, \url{https://scivideos.org/pirsa/14080000}}
          }
          

Prajval Shastri Indian Institute of Astrophysics

Source Repository PIRSA
Talk Type Scientific Series
Subject

Abstract

Accreting supermassive black holes in the centres of galaxies (i.e. Active Galactic Nuclei - AGN) are now known to play a prominent role in the growth of galaxies through cosmic time. The fundamental parameters to explain the whole range of observed properties of these accreting systems, however, is still elusive. We will present some results from multi-wavelength investigations of the nature of accreting supermassive black holes, including those that produce low kinetic power jets as well as high kinetic power, relativistic jets.