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astro-ph2005
Hydrogen Burning of 17-O in Classical Novae
A. Chafa, V. Tatischeff, P. Aguer +10
We report on the observation of a previously unknown resonance at E=194.1+/-0.6 keV (lab) in the 17-O(p,alpha)14-N reaction, with a measured resonance strength omega_gamma(p,alpha)…
astro-ph2003
Reevaluation of the Na(p,) reaction rate: Implications for the detection of Na gamma rays from novae
D. G. Jenkins, C. J. Lister, R. V. F. Janssens +8
Understanding the processes which create and destroy Na is important for diagnosing classical nova outbursts. Conventional Na(p,) studies are complicated by the ne…