Three routes to jet collimation by the Balbus-Hawley magnetorotational instability

Monthly Notices of the Royal Astronomical Society

Volumn 361, Issue 1, 2005, Pages 345-356

  Williams, Peter T ^a,b,c  

^a City College of San Francisco ^*  (United States)

^b CITY COLLEGE OF SAN FRANCISCO   (United States)

^c LOS ALAMOS NATIONAL LABORATORY   (United States)

Author keywords

Accretion, accretion discs; Galaxies: jets; MHD; Polarization; Stars: winds, outflows; Turbulence

Indexed keywords

FIGHTER AIRCRAFT; GAMMA RAYS; MAGNETOHYDRODYNAMICS; RESIDUAL STRESSES; TURBULENCE;

ACCRETION FLOW; ACCRETION: ACCRETION DISKS; CORE COLLAPSE; DISPERSION RELATIONS; GALAXIES JETS; HOOP STRESS; MAGNETOHYDRODYNAMIC TURBULENCE; MAGNETOROTATIONAL INSTABILITY; STARS: WINDS OUTFLOWS; VISCOELASTICS;

POLARIZATION;

EID: 22944476130     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2005.08906.x     Document Type: Article

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