Interaction of Gravitationally Contracting Gas Having Angular Momentum with Magnetic Field, and the Acceleration and Collimation of Astrophysical Jets

Details Interaction of Gravitationally Contracting Gas Having Angular Momentum with Magnetic Field, and the Acceleration and Collimation of Astrophysical Jets Interaction of Gravitationally Contracting Gas Having Angular Momentum with Magnetic Field, and the Acceleration and Collimation of Astrophysical Jets

May 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000iaus..195..213u&link_type=abstract

Highly Energetic Physical Processes and Mechanisms for Emission from Astrophysical Plasmas, Proceedings of IAU Symposium #195, h

Astronomy and Astrophysics

Astrophysics

4

Scientific paper

In the present paper, we stress the importance of the magnetic field in the problem of acceleration and collimation of astrophysical jets, and discuss our proposed generic picture for such ``central gravitator + jets + lobes" systems and inherent interpretations of the various observational characteristics of such systems: Mechanisms are proposed for (1) the enhanced liberation of gravitational energy at the central object, (2) the transfer of a part of the liberated energy along the large-scale magnetic field by large-amplitude, torsional Alfven wave trains that form collimated jets (we call this a sweeping pinch process), (3) the dumping of the transferred energy at the end of the jets when they impinge on the denser region outside the border of the ``cavity" from which the mass contracted to the central condensation (central gravitator + accretion disk, as well as the larger-scale condensation surrounding them), and (4) the formation of wiggled jets and lobes as helical kinks and the tucked-up magnetic field produced in the sweeping pinch process, respectively.

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