On Radiative Acceleration of Jets and Outflows from Advective Disks
Astrophysics
2009-10-31 v1
Abstract
Jets and outflows are known to form out of advective accretion flows around black holes. Hard photons from the centrifugal barrier directly hit the electrons and deposit momentum on them. For optically thick flows such deposition is not efficient, but for optically thin flows matter could be accelerated to relativistic speed. In fact, even bound matter could be made free through successive deposition. We discuss these possibilities.
Cite
@article{arxiv.astro-ph/0012534,
title = {On Radiative Acceleration of Jets and Outflows from Advective Disks},
author = {Indranil Chattopadhyay and Sandip K. Chakrabarti},
journal= {arXiv preprint arXiv:astro-ph/0012534},
year = {2009}
}
Comments
AIP Publication, Macro included