A note on the validity of the use of Euler's equation for the motion of the matter in the envelopes of Be stars

Details A note on the validity of the use of Euler's equation for the motion of the matter in the envelopes of Be stars A note on the validity of the use of Euler's equation for the motion of the matter in the envelopes of Be stars

Mar 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975ap%26ss..33...99m&link_type=abstract

Astrophysics and Space Science, vol. 33, Mar. 1975, p. 99-101.

Astronomy and Astrophysics

Astrophysics

1

B Stars, Euler Equations Of Motion, Mass Transfer, Stellar Envelopes, Angular Velocity, Astronomical Models, Boltzmann Transport Equation, Hydrodynamic Equations, Ideal Fluids, Molecular Collisions, Stellar Structure

Scientific paper

Three assumptions which underlie the theoretical treatment of the
structure and kinematics of the circumstellar material surrounding Be
stars are examined. It is shown that a single-fluid non-viscous
hydrodynamical description is a reasonable one for describing the motion
of a fluid under typical envelope conditions

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