Stellar reaction rate of 14N(p, γ)15O and hydrogen burning in massive stars☆
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Supported in part by the Deutsche Forschungsgemeinschaft (Ro 429/13-3 and Ro 429/15-1), the Friedrich Flick Förderungsstiftung and the Natural Sciences and Engineering Research Council of Canada.
- 1
Permanent address: CNRS, Batiment 104, 91406 ORSAY, France.
- 2
Present address: Department of Physics, University of Notre Dame, Notre Dame, Indiana, USA.
Copyright © 1987 Published by Elsevier B.V.