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The reaction rates of neutron capture reactions on light nuclei are importantfor reliably simulating nucleosynthesis in a variety of stellar scenarios.Neutron capture reaction rates on neutron-rich C-, N-, and O-isotopes arecalculated in the framework of a hybrid compound and direct capture model. Theresults are tabulated and compared with the results of previous calculations aswell as with experimental results.Comment: 33 pages (uses revtex) and 9 postscript figures, accepted for  publication in Phys. Rev.

Reaction rates for neutron capture reactions to C, N, and O isotopes to the neutron rich side of stability