Hollow conical jet models for SS 433 - A paradigm lost?

Details Hollow conical jet models for SS 433 - A paradigm lost? Hollow conical jet models for SS 433 - A paradigm lost?

Feb 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990apj...350..561k&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 350, Feb. 20, 1990, p. 561-577.

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Computation

18

Astronomical Models, Computational Astrophysics, Eclipsing Binary Stars, Radio Jets (Astronomy), Bow Waves, Emission Spectra, Finite Difference Theory, Precession, Shock Waves, Supernova Remnants

Scientific paper

A precessing jet such as that in SS 433 may be approximated as an axisymmetric flow, if the precession time is short by comparison to the propagation time. A series of simulations has been conducted for precessing jets using an axisymmetric finite-difference hydrodynamics code. Examinations are made of hollow cylindrical jets, which lack the complication of a growing interior volume, and conical jets, which model the behavior of a precessing jet propagating on the surface of its precession cone.

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