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. https://pirsa.org/14080000
MLA
Shastri, Prajval. Probing the Physics of Active Galaxies Using Multi-wavelength Data. Perimeter Institute, Aug. 05, 2014, https://pirsa.org/14080000
BibTex
@misc{ pirsa_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}, year = {2014}, month = {aug}, note = {PIRSA:14080000 see, \url{https://pirsa.org}} }
Indian Institute of Astrophysics
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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.