Interaction of Jets with Galactic Winds

M. Krause; M. Camenzind

doi:10.1007/3-540-26589-9_8

Interaction of Jets with Galactic Winds

M. Krause, M. Camenzind

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

Abstract

We have used the vectorised and parallelised magnetohydrodynamics code NIRVANA on the NEC SX-5 and the new SX-6 installation in parallel mode to simulate the interaction of jets with a galactic wind that might be typical for the star-bursting radio-galaxies of the early universe.

Original language	Undefined/Unknown
Title of host publication	High Performance Computing in Science and Engineering '04, eds.: Krause,~E. and Jäger,~W. and Resch,~M., Springer
Editors	E. Krause, W. Jager, M. Resch
Publisher	Springer Nature
ISBN (Electronic)	978-3-540-26589-4
ISBN (Print)	978-3-540-22943-8
DOIs	https://doi.org/10.1007/3-540-26589-9_8
Publication status	Published - 2004

Access to Document

10.1007/3-540-26589-9_8

Cite this

@inproceedings{df1252d1d34f4858bd52c342e27a3ce2,

title = "Interaction of Jets with Galactic Winds",

abstract = "We have used the vectorised and parallelised magnetohydrodynamics code NIRVANA on the NEC SX-5 and the new SX-6 installation in parallel mode to simulate the interaction of jets with a galactic wind that might be typical for the star-bursting radio-galaxies of the early universe.",

author = "M. Krause and M. Camenzind",

year = "2004",

doi = "10.1007/3-540-26589-9_8",

language = "Undefined/Unknown",

isbn = "978-3-540-22943-8",

editor = "E. Krause and W. Jager and M. Resch",

booktitle = "High Performance Computing in Science and Engineering '04, eds.: Krause,~E. and J{\"a}ger,~W. and Resch,~M., Springer",

publisher = "Springer Nature",

address = "Netherlands",

}

TY - GEN

T1 - Interaction of Jets with Galactic Winds

AU - Krause, M.

AU - Camenzind, M.

PY - 2004

Y1 - 2004

N2 - We have used the vectorised and parallelised magnetohydrodynamics code NIRVANA on the NEC SX-5 and the new SX-6 installation in parallel mode to simulate the interaction of jets with a galactic wind that might be typical for the star-bursting radio-galaxies of the early universe.

AB - We have used the vectorised and parallelised magnetohydrodynamics code NIRVANA on the NEC SX-5 and the new SX-6 installation in parallel mode to simulate the interaction of jets with a galactic wind that might be typical for the star-bursting radio-galaxies of the early universe.

U2 - 10.1007/3-540-26589-9_8

DO - 10.1007/3-540-26589-9_8

M3 - Conference contribution

SN - 978-3-540-22943-8

BT - High Performance Computing in Science and Engineering '04, eds.: Krause,~E. and Jäger,~W. and Resch,~M., Springer

A2 - Krause, E.

A2 - Jager, W.

A2 - Resch, M.

PB - Springer Nature

ER -