Search Results - (Author, Cooperation:V. V. Gvaramadze)
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1J. Mackey ; S. Mohamed ; V. V. Gvaramadze ; R. Kotak ; N. Langer ; D. M. Meyer ; T. J. Moriya ; H. R. Neilson
Nature Publishing Group (NPG)
Published 2014Staff ViewPublication Date: 2014-08-15Publisher: Nature Publishing Group (NPG)Print ISSN: 0028-0836Electronic ISSN: 1476-4687Topics: BiologyChemistry and PharmacologyMedicineNatural Sciences in GeneralPhysicsPublished by: -
2Gvaramadze, V. V. ; Lominadze, J. G. ; Ruzmaikin, A. A. ; Sokoloff, D. d. ; Shukurov, A. M.
Springer
Published 1988Staff ViewISSN: 1572-946XSource: Springer Online Journal Archives 1860-2000Topics: PhysicsNotes: Abstract We consider evolution of the regular magnetic field in turbulent astrophysical jets. The observed lateral expansion of a jet is approximately described by a linear in coordinates regular velocity field (the Hubble flow). It is shown that in expanding turbulent jets with non-vanishing mean helicity of the turbulence temporal amplification and effective realignment of the regular magnetic field occurs with the field changing orientation from the transverse to the longitudinal one along the jet axis. The distance at which the realiggment occurs depends on parameters of the jet, in particular, on the power of the central source. Estimates for the jet in a weak source 3C 31 favourably agree with observations.Type of Medium: Electronic ResourceURL: -
3Staff View
ISSN: 1573-8191Source: Springer Online Journal Archives 1860-2000Topics: PhysicsType of Medium: Electronic ResourceURL: -
4Staff View
ISSN: 1572-946XKeywords: Neutron stars ; Unsteady accretion ; GRBsSource: Springer Online Journal Archives 1860-2000Topics: PhysicsNotes: Abstract We propose a model of gamma-ray bursts (GRBs) based on close Galactic neutron stars with accretion disks. We outline a simple mechanism of unsteady plasma ejections during episodic accretion events. The relative kinetic energy of ejected blobs can be converted into gamma-rays by internal shocks. The beaming of gamma-ray emission can be responsible for the observed isotropic angular distribution of GRBs.Type of Medium: Electronic ResourceURL: