Terminal Outflow Velocities from the Mass-Losing AGB Stars

Details Terminal Outflow Velocities from the Mass-Losing AGB Stars Terminal Outflow Velocities from the Mass-Losing AGB Stars

Jul 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997ap%26ss.251..231k&link_type=abstract

Astrophysics and Space Science, Volume 251, Issue 1-2, pp. 231-234

Astronomy and Astrophysics

Astrophysics

Scientific paper

We have calculated terminal gas outflow velocities from the circumstellar shells of the AGB stars. Our results confirm that, in case of the stationary dust driven winds, the dynamics of the outflow is governed essentially by the dust properties and stellar luminosities, while only marginally by other stellar parameters. Although being far from comprehensive, our calculations also indicate that the dust driven winds may only occur in cool, luminous, low mass objects.

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