Stability of Massive Stars and the Humphreys / Davidson Limit

Details Stability of Massive Stars and the Humphreys / Davidson Limit Stability of Massive Stars and the Humphreys / Davidson Limit

Jul 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993mnras.263..375g&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Vol. 263, NO.2/JUL15, P. 375, 1993

Other

53

Instabilities - Stars: Oscillations - Stars: Supergiants - Stars: Variables: Other

Scientific paper

Using standard physics and opacities, the stability of massive stars is
re-examined. Violent mode-coupling instabilities are identified which
could account for the LBV phenomenon. The stability boundary seems to be
related to the Humphreys-Davidson limit.

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