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Measurement of alpha‐widths in 16O relevant to astrophysics

dc.contributor.authorBecchetti, Fredrick D.en_US
dc.contributor.authorJanecke, Joachimen_US
dc.contributor.authorOverway, D. J.en_US
dc.contributor.authorThorn, C. E.en_US
dc.contributor.authorFlynn, E. R.en_US
dc.contributor.authorHanson, D. L.en_US
dc.contributor.authorSunier, J. W.en_US
dc.contributor.authorKekelis, G.en_US
dc.date.accessioned2011-11-15T16:01:25Z
dc.date.available2011-11-15T16:01:25Z
dc.date.issued1978-12-01en_US
dc.identifier.citationBecchetti, F. D.; Janecke, J.; Overway, D.; Thorn, C.; Flynn, E. R.; Hanson, D. L.; Sunier, J. W.; Kekelis, G. (1978). "Measurement of alpha‐widths in 16O relevant to astrophysics." AIP Conference Proceedings 47(1): 752-753. <http://hdl.handle.net/2027.42/87457>en_US
dc.identifier.urihttps://hdl.handle.net/2027.42/87457
dc.description.abstractSeveral different α‐transfer reactions, 12C→16O, have been studied at high bombarding energies with magnetic spectrometers. Line‐widths, α‐spectroscopic factors, Sα, and reduced α‐widths, γα2 and ϑα2, have been determined for levels in 16O, including several of importance in astrophysics.en_US
dc.publisherThe American Institute of Physicsen_US
dc.rights© The American Institute of Physicsen_US
dc.titleMeasurement of alpha‐widths in 16O relevant to astrophysicsen_US
dc.typeArticleen_US
dc.subject.hlbsecondlevelPhysicsen_US
dc.subject.hlbtoplevelScienceen_US
dc.description.peerreviewedPeer Revieweden_US
dc.contributor.affiliationumUniversity of Michigan, Ann Arbor, Mi. 48109en_US
dc.contributor.affiliationotherBrookhaven National Laboratory, Upton, L. I., NY 11973en_US
dc.contributor.affiliationotherLASL, Los Alamos, N. M. 47544en_US
dc.contributor.affiliationotherWilliams College, Williamstown, Ma. 01267en_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/87457/2/752_1.pdf
dc.identifier.doi10.1063/1.31585en_US
dc.identifier.sourceAIP Conference Proceedingsen_US
dc.owningcollnamePhysics, Department of


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