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Description
  • Runaway instability operates in fluid tori around black holes. It affects systems close to the critical (cusp overflowing) configuration. The runaway effect depends on the radial profile l(R) of the angular momentum distribution of the fluid, on the dimension-less spin a of the central black hole (|a| 1), and other factors, such as self-gravity.
  • Runaway instability operates in fluid tori around black holes. It affects systems close to the critical (cusp overflowing) configuration. The runaway effect depends on the radial profile l(R) of the angular momentum distribution of the fluid, on the dimension-less spin a of the central black hole (|a| 1), and other factors, such as self-gravity. (en)
Title
  • Effect of the toroidal magnetic field on the runaway instability of relativistic tori
  • Effect of the toroidal magnetic field on the runaway instability of relativistic tori (en)
skos:prefLabel
  • Effect of the toroidal magnetic field on the runaway instability of relativistic tori
  • Effect of the toroidal magnetic field on the runaway instability of relativistic tori (en)
skos:notation
  • RIV/67985815:_____/13:00393329!RIV14-GA0-67985815
http://linked.open...avai/riv/aktivita
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  • I, P(GC13-00070J)
http://linked.open...iv/cisloPeriodika
  • July
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  • 71809
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  • RIV/67985815:_____/13:00393329
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  • accretion; accretion disks; black hole physics (en)
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http://linked.open...odStatuVydavatele
  • FR - Francouzská republika
http://linked.open...ontrolniKodProRIV
  • [464997CBBC39]
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  • Astronomy & Astrophysics
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  • 555
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  • Karas, Vladimír
  • Hamerský, Jaroslav
http://linked.open...ain/vavai/riv/wos
  • 000322008600032
issn
  • 0004-6361
number of pages
http://bibframe.org/vocab/doi
  • 10.1051/0004-6361/201321500
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