Importance of the continuous nuclear spectrum for the thermal post-main sequence evolution of a 6 solar-mass star

Details Importance of the continuous nuclear spectrum for the thermal post-main sequence evolution of a 6 solar-mass star Importance of the continuous nuclear spectrum for the thermal post-main sequence evolution of a 6 solar-mass star

Jun 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977a%26a....58..445s&link_type=abstract

Astronomy and Astrophysics, vol. 58, no. 3, June 1977, p. 445-447.

Astronomy and Astrophysics

Astrophysics

3

Continuous Spectra, Stellar Evolution, Stellar Models, Stellar Spectra, Chemical Composition, Computerized Simulation, Eigenvectors, Fourier Analysis, Hertzsprung-Russell Diagram, Secular Variations, Stability Tests

Scientific paper

A 6 solar-mass in the phase of crossing the Hertzsprung gap is subjected to a secular stability analysis, including a perturbation of chemical abundances. Both the usual secular spectrum and the continuous nuclear spectrum are found in the numerical computations. The slowest (real) mode of the continuous nuclear spectrum contributes considerably to the evolution, especially of the core and shell source regions.

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