Synthesis of radioactive nuclei and the annihilation line from novae

Details Synthesis of radioactive nuclei and the annihilation line from novae Synthesis of radioactive nuclei and the annihilation line from novae

Apr 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000aipc..510..102c&link_type=abstract

THE FIFTH COMPTON SYMPOSIUM. AIP Conference Proceedings, Volume 510, pp. 102-106 (2000).

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Nucleosynthesis In Novae, Supernovae, And Other Explosive Environments, Novae, Dwarf Novae, Recurrent Novae, And Other Cataclysmic Variables, Elementary Particle Processes, Stellar Structure, Interiors, Evolution, Nucleosynthesis, Ages

Scientific paper

A possible range of the abundance of radioactive nuclei in CO and ONeMg nova ejecta was found via kinetic computations of the thermonuclear burning in the one-zone hydrogen-rich envelope. We calculate the light curve of the annihilation line for various conditions and found that the principal parameter responsible for the uncertainty of the predicted flux is the mixing degree. The annihilation line observations of 18F and an independent estimate of the total amount of synthesised 18F from 18O may be used to assess the mixing degree of radioactive nuclei in the envelope. .

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