The role of the magnetic field in gas-dust coupling in late-type stellar winds

Details The role of the magnetic field in gas-dust coupling in late-type stellar winds The role of the magnetic field in gas-dust coupling in late-type stellar winds

Aug 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994ap%26ss.218...23h&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 218, no. 1, p. 23-28

Computer Science

Numerical Analysis

6

Cosmic Dust, Coupling, Gas Dynamics, Late Stars, Magnetic Field Configurations, Magnetization, Radiation Distribution, Radiation Pressure, Stellar Envelopes, Stellar Magnetic Fields, Stellar Winds, Coronal Holes, Equations Of Motion, Mathematical Models, Numerical Analysis

Scientific paper

We show that the existence of anchored magnetic loops in the envelopes
of evolved late-type stars would guarantee that the grains in
radiatively driven winds would remain well-coupled to the neutral gas.

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