A multi-fluid model for stellar winds

Details A multi-fluid model for stellar winds A multi-fluid model for stellar winds

Jun 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977cosp.meetq....m&link_type=abstract

COSPAR, Plenary Meeting, 20th, Tel Aviv, Israel, June 7-18, 1977, Paper. 14 p.

Other

Astronomical Models, Flow Theory, Magnetohydrodynamic Flow, Stellar Winds, Critical Point, Flow Equations, Flow Velocity, Two Fluid Models

Scientific paper

A multi-fluid model describing the time-independent plasma flow in stellar winds is formulated. This plasma includes electrons and different types of ions which are allowed to have different streaming velocities as well as different nonisothermal temperatures. This flexibility means that the various energy equations are explicitly incorporated in the model. Analytical explicit expressions for the ion momentum equations make it possible to analyze the various conditions for the critical points even in this complicated multi-fluid case.

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