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Astron. Astrophys. 328, 107-120 (1997)

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Acknowledgements

We wish to thank R. Lehoucq warmly for his first version of the code that we used to calculate the nuclear reaction rates. We also thank Reuven Ramaty for details on the unresolved gamma-ray lines. We are grateful to Jurgen Kiener for providing us with accurate tables of energy loss rates. This work has been done in the framework of the PICS `Nuclear gamma-ray lines and associated nucleosynthesis'.

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© European Southern Observatory (ESO) 1997

Online publication: March 24, 1998

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