Other
Scientific paper
May 1999
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999apj...516..366s&link_type=abstract
The Astrophysical Journal, Volume 516, Issue 1, pp. 366-368.
Other
12
Stars: Individual (P Cygni), Stars: Oscillations, Stars: Variables: Other (Luminous Blue Variables)
Scientific paper
By employing as input parameters only observationally determined stellar surface quantities, detailed envelope models for six well-observed luminous blue variables at quiescence are constructed and tested for marginal dynamical instability. The best-observed of these objects, P Cyg, proves to be exactly in a state of marginal dynamical instability, just as predicted. Within the larger observational errors estimated for the five other objects, they too are probably in the same marginally unstable state as P Cyg.
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