Vladimir I. Pariev, Ph.D. - Publications
Affiliations: | 2001 | University of Arizona, Tucson, AZ |
Area:
Astronomy and AstrophysicsYear | Citation | Score | |||
---|---|---|---|---|---|
2012 | Beskin VS, Zheltoukhov AA, Pariev VI. An accretion disk without angular momentum near a black hole Astronomy Reports. 56: 1-8. DOI: 10.1134/S1063772912010015 | 0.313 | |||
2007 | Pariev VI, Colgate SA, Finn JM. A magnetic α-ω dynamo in AGN disks. II. Magnetic field generation, theories, and simulations Astrophysical Journal. 658: 129-160. DOI: 10.1086/510735 | 0.402 | |||
2007 | Pariev VI, Colgate SA. A magnetic α-ω dynamo in AGN disks. I. The hydrodynamics of star-disk collisions and keplerian flow Astrophysical Journal. 658: 114-128. DOI: 10.1086/510734 | 0.404 | |||
2005 | Lyutikov M, Pariev VI, Gabuzda DC. Polarization and structure of relativistic parsec-scale AGN jets Monthly Notices of the Royal Astronomical Society. 360: 869-891. DOI: 10.1111/j.1365-2966.2005.08954.x | 0.321 | |||
2003 | Lyutikov M, Pariev VI, Blandford RD. Polarization of prompt gamma-ray burst emission: Evidence for electromagnetically dominated outflow Astrophysical Journal. 597: 998-1009. DOI: 10.1086/378497 | 0.307 | |||
2003 | Pariev VI, Istomin YN, Beresnyak AR. Relativistic parsec-scale jets: II. Synchrotron emission Astronomy and Astrophysics. 403: 805-816. | 0.354 | |||
1998 | Pariev VI, Bromley BC. Line emission from an accretion disk around a black hole: Effects of disk structure Astrophysical Journal. 508: 590-600. DOI: 10.1086/306420 | 0.544 | |||
1998 | Bromley BC, Miller WA, Pariev VI. The inner edge of the accretion disk around a supermassive black hole Nature. 391: 54-56. DOI: 10.1038/34130 | 0.531 | |||
1996 | Istomin YN, Pariev VI. Stability of a relativistic rotating electron-positron jet: Non-axisymmetric perturbations Monthly Notices of the Royal Astronomical Society. 281: 1-26. | 0.347 | |||
1996 | Pariev VI. Hydrodynamic accretion on to a rapidly rotating Kerr black hole Monthly Notices of the Royal Astronomical Society. 283: 1264-1280. | 0.324 | |||
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