Cool Evolved Winds: Use of the Eclipsing Technique

Details Cool Evolved Winds: Use of the Eclipsing Technique Cool Evolved Winds: Use of the Eclipsing Technique

Jun 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aspc..425..191c&link_type=abstract

Hot and Cool: Bridging Gaps in Massive Star Evolution ASP Conference Series Vol. 425, Proceedings of a Workshop held at the Cali

Astronomy and Astrophysics

Astronomy

Scientific paper

For those red giants and supergiants which do not exhibit an optically thick circumstellar dust shell, the observation of massive stellar winds remains an outstanding problem. The wind-driving mechanism, as well as many wind characteristics through the wind-acceleration region, are unknown. We discuss the use of eclipsing binary systems to analyze the important regions at the base of the outflow, with reference to work we have carried out on a small sample of red giants in symbiotic binary systems.

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