On Radiative Acceleration of Jets and Outflows from Advective Disks

Details On Radiative Acceleration of Jets and Outflows from Advective Disks On Radiative Acceleration of Jets and Outflows from Advective Disks

2000-12-29

arxiv.org/abs/astro-ph/0012534v1

Astronomy and Astrophysics

Astrophysics

AIP Publication, Macro included

Scientific paper

10.1063/1.1370888

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.

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