Massive Stellar Interiors and the Hot/Cool Star Connection

Details Massive Stellar Interiors and the Hot/Cool Star Connection Massive Stellar Interiors and the Hot/Cool Star Connection

May 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aas...210.4006y&link_type=abstract

American Astronomical Society Meeting 210, #40.06; Bulletin of the American Astronomical Society, Vol. 39, p.154

Physics

Scientific paper

Very massive stars undergo excursions to both blue and red extremes of the HR Diagram. New desciptions of stellar interior physics and evolution including hydrodynamic processes result in substantial differences in structure from traditional stellar models. In particular, massive compact cores can drive stars to red extremes that are unstable to eruptive phenomena. I will discuss evolution calculations and prelimiary multi-D simulations with radiative transfer for massive stars at the hot/cool star boundary.

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