Magnetic field upper limits for jet formation
نویسندگان
چکیده
منابع مشابه
Magnetic Field Upper Limits for Jet Formation
Context. Very high magnetic fields at the surface of neutron stars or in the accretion disk of black holes inhibit the production of jets. Aims. We quantify here the magnetic field strength for the jet formation. Methods. By using, the Alfvén Radius, RA, we study what we call the basic condition, RA/R∗ = 1 or RA/RLSO = 1 (LSO, last stable orbit), in its dependency with the magnetic field streng...
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ژورنال
عنوان ژورنال: Astronomy & Astrophysics
سال: 2007
ISSN: 0004-6361,1432-0746
DOI: 10.1051/0004-6361:20077567