The treatment of highly non-adiabatic, non-radial...

Monthly Notices of the Royal Astronomical Society 1992 / 05 Vol. 256; Iss. 2

The treatment of highly non-adiabatic, non-radial pulsations by application of the Riccati method to the example of hydrogen-deficient carbon stars

Glatzel, W., Gautschy, A.
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Volume:
256
Journal:
Monthly Notices of the Royal Astronomical Society
DOI:
10.1093/mnras/256.2.209
Date:
May, 1992
File:
PDF, 215 KB
1992
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