Effects of a Clumpy Circumstellar Medium on the Dynamics of Stellar Winds

Details Effects of a Clumpy Circumstellar Medium on the Dynamics of Stellar Winds Effects of a Clumpy Circumstellar Medium on the Dynamics of Stellar Winds

Feb 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995ap%26ss.224..423a&link_type=abstract

Astrophysics and Space Science, Volume 224, Issue 1-2, pp. 423-424

Astronomy and Astrophysics

Astrophysics

Hydrodynamics, Stars: Mass-Loss, Ism: Kinematics And Dynamics, Planetary Nebulae

Scientific paper

Mass pickup from clumps resulting from previous mass loss phases by a
fast stellar wind can substantially modify its behaviour, even leading
to a highly supersonic wind becoming transonic before leaving the
mass-loading region. The observational consequences of mass-loading on
these astrophysical flows is discussed.

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