Carbburnnuclat.pdf

spc_stnv_000189

"Carbon-Burning Nucleosynthesis at Constant Temperature."

OAP-144

"Carbon-Burning Nucleosyntesis at Constant Temperature" is part of the Orange Aid preprint Series in Nuclear Astrophysics, August 1968. The abstract states "Syntesis of elements during thermonuclear burning of carbon is examined at a series of temperatures (T=0.6, 0.8, 1.0, 1.2, 1.4) and for several initial compositions. Recent eperimental results (Ptterson, Winkler, and Zaidins 1968) for the 12C+!@C reaction are used. A general method for numerical solution of nuclear-reaction networkds is described. At the higher temperatures in the range now thought to be appropriate for carbon burning in stars,

1968-08-01

Saturn V Collection

Box 27, Folder 41

University of Alabama in Huntsville Archives, Special Collections, and Digital Initiatives, Huntsville, Alabama

Orange Aid Preprint Series in Nuclear Astrophysics

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