The secular and thermal spectrum of hydrogen-deficient carbon stars

Details The secular and thermal spectrum of hydrogen-deficient carbon stars The secular and thermal spectrum of hydrogen-deficient carbon stars

Dec 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991mnras.253..509g&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 253, Dec. 1, 1991, p. 509-521.

Astronomy and Astrophysics

Astronomy

5

Carbon Stars, Secular Variations, Stellar Oscillations, Stellar Spectra, B Stars, Hydrogen

Scientific paper

Applying the Riccati method to the secular problem, secular and thermal spectra of a 0.9 solar mass HdC star are investigated in various evolutionary phases. The onset of shell burning is associated with a bewildering complexity of the thermal and secular spectrum and is interpreted using a simplified analytical model. Shell burning leads to the decoupling of different parts of the spectrum, one of which seems to be closely related to the strange mode II phenomenon.

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