Astronomy and Astrophysics – Astrophysics
Scientific paper
Feb 1977
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977apj...212..159s&link_type=abstract
Astrophysical Journal, Part 1, vol. 212, Feb. 15, 1977, p. 159-170.
Astronomy and Astrophysics
Astrophysics
24
Periodic Variations, Radiation Pressure, Stellar Evolution, Stellar Models, Stellar Structure, Thermonuclear Reactions, Astrophysics, Equations Of State, Helium, Quenching (Cooling), Stellar Mass
Scientific paper
An analysis is conducted of a typical stellar helium shell flash cycle. A sequence of 12 flashes for a population I star is considered. The changes taking place at a constant mass layer in the helium-burning shell are studied as the flash develops. A highly simplified mathematical description is presented, taking into account the three necessary conditions for the occurrence of the flash and the pressure-density and temperature-density relationships. Quantities which are helpful in explaining what triggers the flash are found to be useful in explaining what quenches the flash.
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