O the Dynamical Structure of the Jet System in the Disk with the Keplerian Rotation

Details O the Dynamical Structure of the Jet System in the Disk with the Keplerian Rotation O the Dynamical Structure of the Jet System in the Disk with the Keplerian Rotation

Jun 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989jass....6...17j&link_type=abstract

Journal of Astronomy and Space Sciences, vol.6, no1, p.17-28

Astronomy and Astrophysics

Astronomy

Scientific paper

The classical sloar wind theory proposed by Parker(1963) explains well the dynamics of the wind pheonomena such as stellar wind accretion disk. While the stellar wind system like the solar wind has the spherically symmetric wind structure, there are various jet phenomena which collimate the system into the narrow space. We can find these dynamical structures in SS433, in the optical jet of M87, and around the active galactic nulei. We present the dynamical structure of the jet system in disks, which conserves the angular momentum, with the Keplerian rotation and the strong relation between the geometrical cross section and the physical change of the jet stream on the basis of the hydrodynamic equations.

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