Viscous kelvin-helmholtz instabilities in highly ionized plasmas

Monthly Notices of the Royal Astronomical Society

Volumn 436, Issue 2, 2013, Pages 1721-1740

  Roediger, E ^a,b,c   Kraft, R P ^c   Nulsen, P ^c   Churazov, E ^d   Forman, W ^c   Bruggen M ^a   Kokotanekova, R ^b,c,e  

^a UNIVERSITY OF HAMBURG   (Germany)

^b JACOBS UNIVERSITY BREMEN   (Germany)

^c HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^d MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

^e UNIVERSITY OF INNSBRUCK   (Austria)

Author keywords

Galaxies: clusters: intracluster medium; Hydrodynamics; Instabilities; Methods: numerical; Plasmas; X rays: galaxies: clusters.

Indexed keywords

BUOYANCY; GALAXIES; LONG TERM EVOLUTION (LTE); MIXING; PLASMA DIAGNOSTICS; PLASMA STABILITY; REYNOLDS NUMBER; SHEAR FLOW; VISCOSITY;

GALAXIES: CLUSTERS: INTRACLUSTER MEDIUMS; HIGHLY-IONIZED; IONIZED PLASMAS; KELVIN- HELMHOLTZ INSTABILITIES; METHOD: NUMERICAL; SPITZER; TEMPERATURE DEPENDENT; TRANSPORT COEFFICIENT; X-RAY: GALAXY: CLUSTER.; X-RAYS GALAXIES CLUSTERS;

NUMERICAL METHODS;

EID: 84888044935     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1093/mnras/stt1691     Document Type: Article

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