Steady stellar jets

Details Steady stellar jets Steady stellar jets

Apr 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987mnras.225..741f&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 225, April 1, 1987, p. 741-759. Research supported by t

Astronomy and Astrophysics

Astronomy

57

Late Stars, Radiant Cooling, Steady Flow, Stellar Models, Stellar Winds, Supersonic Jet Flow, Gas Dynamics, Oxygen

Scientific paper

This paper contains some results of axisymmetric numerical calculations of the shock structures in steady supersonic jets in which there is significant radiative cooling. It is found that the regularly spaced shock cells found in adiabatic jets still occur and that cooling can by itself induce shocks if it is fast enough. The forbidden O I line emission from such jets is calculated and compared to that seen in stellar jets. The pattern of emission is very similar to that observed, which suggests that a number of the features of stellar jets can be understood in this way.

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