3d grmhd simulations of disk-jet coupling and emission - INSPIRE

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3d grmhd simulations of disk-jet coupling and emission

Ken-Ichi Nishikawa
(
- USRA, Huntsville
)
,
Y. Mizuno
(
- USRA, Huntsville
)
,
S. Fuerst
(
- Mullard Space Sci. Lab.
)
,
K. Wu
(
- Mullard Space Sci. Lab.
)
,
P. Hardee
(
- Alabama U.
)

Sep, 2005

4 pages

Part of Astrophysical sources of high-energy particles and radiation : Proceedings, Torun, Poland, 20-24 June 2005, 184

Published in:

AIP Conf.Proc. 801 (2005) 1, 184

Contribution to:

Conference on Astrophysical Sources of High Energy Particles and Radiation, 184

Published: Nov 29, 2005

e-Print:

astro-ph/0509601 [astro-ph]

DOI:

10.1063/1.2141858

View in:

ADS Abstract Service

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Abstract: (AIP)

We have also calculated the free‐free emission from a disk/outflow near a rotating black hole using our axisymmetric GRMHD simulation using a covariant radiative transfer formulation. Our calculation shows radiation from a shock, and hence the disk‐jet coupling region is observable.

95.75.Pq
95.30.Qd
97.60.Lf
98.62.Nx
black holes
accretion disks
astrophysical jets
magnetohydrodynamics
computer aided analysis

References(17)

Figures(0)

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