Hot CNO-Ne cycle hydrogen burning - Explosive hydrogen burning in novae

Details Hot CNO-Ne cycle hydrogen burning - Explosive hydrogen burning in novae Hot CNO-Ne cycle hydrogen burning - Explosive hydrogen burning in novae

Mar 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979apj...228..875l&link_type=abstract

Astrophysical Journal, Part 1, vol. 228, Mar. 15, 1979, p. 875-880.

Astronomy and Astrophysics

Astrophysics

24

Astrophysics, Hydrogen, Novae, Nuclear Fusion, Abundance, Carbon, Convective Heat Transfer, Neon, Nitrogen, Stellar Models

Scientific paper

We have studied element production occurring in novae where hydrogen burning proceeds at high temperature on short time scales. We present the results of network computations performed for temperature-density profiles extracted from hydrodynamic studies of these events. We find that, in some cases, a small change in the freeze-out profiles can induce substantial changes in the emerging abundance configurations. The influence of convective mixing and of variations in the initial composition is also found to be important. Implications for the production of the rarer CNO isotopes are discussed.

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