Vladimir I. Pariev, Ph.D.
Affiliations: | 2001 | University of Arizona, Tucson, AZ |
Area:
Astronomy and AstrophysicsGoogle:
"Vladimir Pariev"Mean distance: 4517.33
Parents
Sign in to add mentorJ R. Jokipii | grad student | 2001 | University of Arizona | |
(Magnetic fields: Their origin and manifestation in accretion disks around supermassive black holes.) |
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Publications
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Beskin VS, Zheltoukhov AA, Pariev VI. (2012) An accretion disk without angular momentum near a black hole Astronomy Reports. 56: 1-8 |
Pariev VI, Colgate SA, Finn JM. (2007) A magnetic α-ω dynamo in AGN disks. II. Magnetic field generation, theories, and simulations Astrophysical Journal. 658: 129-160 |
Pariev VI, Colgate SA. (2007) A magnetic α-ω dynamo in AGN disks. I. The hydrodynamics of star-disk collisions and keplerian flow Astrophysical Journal. 658: 114-128 |
Lyutikov M, Pariev VI, Gabuzda DC. (2005) Polarization and structure of relativistic parsec-scale AGN jets Monthly Notices of the Royal Astronomical Society. 360: 869-891 |
Lyutikov M, Pariev VI, Blandford RD. (2003) Polarization of prompt gamma-ray burst emission: Evidence for electromagnetically dominated outflow Astrophysical Journal. 597: 998-1009 |
Pariev VI, Istomin YN, Beresnyak AR. (2003) Relativistic parsec-scale jets: II. Synchrotron emission Astronomy and Astrophysics. 403: 805-816 |
Pariev VI, Bromley BC. (1998) Line emission from an accretion disk around a black hole: Effects of disk structure Astrophysical Journal. 508: 590-600 |
Bromley BC, Miller WA, Pariev VI. (1998) The inner edge of the accretion disk around a supermassive black hole Nature. 391: 54-56 |
Istomin YN, Pariev VI. (1996) Stability of a relativistic rotating electron-positron jet: Non-axisymmetric perturbations Monthly Notices of the Royal Astronomical Society. 281: 1-26 |
Pariev VI. (1996) Hydrodynamic accretion on to a rapidly rotating Kerr black hole Monthly Notices of the Royal Astronomical Society. 283: 1264-1280 |