Effect of Beam-Plasma Instabilities on Accretion Disk Flares

Details Effect of Beam-Plasma Instabilities on Accretion Disk Flares Effect of Beam-Plasma Instabilities on Accretion Disk Flares

2000-02-17

arxiv.org/abs/astro-ph/0002361v1

Astronomy and Astrophysics

Astrophysics

4 pages, 0 figures, accepted for publication in A&A, uses A&A LaTeX macros

Scientific paper

We show that a certain class of flare models for variability from accretion
disk coronae are subject to beam-plasma instabilities. These instabilities can
prevent significant direct acceleration and greatly reduce the variable X-ray
emission argued to arise via inverse Compton scattering involving relativistic
electrons in beams and soft photons from the disk.

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