In this review, analytical results obtained for a wide class of stationary axisymmetric flows in the vicinity of compact astrophysical objects are analyzed, with an emphasis on quantitative predictions for specific sources. Recent years have witnessed a great increase in understanding the formation and properties of astrophysical jets. This is due not only to new observations but also to advances in analytical theory which has produced fairly simple relations, and to what can undoubtedly be called a breakthrough in numerical simulation which has enabled confirmation of theoretical predictions. Of course, we are still very far from fully understanding the physical processes occurring in compact sources. Nevertheless, the progress made raises hopes for near-future test observations that can give insight into the physical processes occurring in active astrophysical objects.

PACS: 95.30.Qd, 97.60.Gb, 97.60.Lf, 98.62.Nx (all) DOI: 10.3367/UFNe.0180.201012b.1241 URL: https://ufn.ru/en/articles/2010/12/b/ 000288495700002 2-s2.0-79955614053 Citation: Beskin V S "Magnetohydrodynamic models of astrophysical jets" Phys. Usp. 53 1199–1233 (2010) BibTexBibNote ® (generic)BibNote ® (RIS) MedlineRefWorks PT Journal Article TI Magnetohydrodynamic models of astrophysical jets AU Beskin V S FAU Beskin VS DP 10 Dec, 2010 TA Phys. Usp. VI 53 IP 12 PG 1199-1233 RX 10.3367/UFNe.0180.201012b.1241 URL https://ufn.ru/en/articles/2010/12/b/ SO Phys. Usp. 2010 Dec 10;53(12):1199-1233 Оригинал: Бескин В С «Магнитогидродинамические модели астрофизических струйных выбросов» УФН 180 1241–1278 (2010); DOI: 10.3367/UFNr.0180.201012b.1241