Origin of the <span class="aps-inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mrow><mmultiscripts><mrow></mrow><mprescripts></mprescripts><mrow></mrow><mrow><mn>13</mn></mrow><mrow></mrow><mrow></mrow></mmultiscripts></mrow></math></span>C<span class="aps-inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mrow><msup><mrow><mo>+</mo></mrow><mrow><mn>17</mn></mrow></msup></mrow></math></span>O resonant structure

R. M. Freeman; Z. Basrak; F. Haas; A. Hachem; G. A. Monnehan; A. Morsad; M. Youlal

doi:10.1103/PhysRevC.38.1081

Origin of the ${}^{13}$ C $+^{17}$ O resonant structure

R. M. Freeman, Z. Basrak, F. Haas, A. Hachem, G. A. Monnehan, A. Morsad, and M. Youlal

Phys. Rev. C 38, 1081 – Published 1 August 1988

Abstract

Using particle techniques, we have been unable to reproduce the resonant structure in the inelastic channel of the ${}^{13}$ C $+^{17}$ O reaction. The structure previously observed in the γ-ray yields for the 0.871-MeV transition is now believed to be due to a hydrogen contamination.

Received 1 March 1988

DOI:https://doi.org/10.1103/PhysRevC.38.1081

Authors & Affiliations

R. M. Freeman, Z. Basrak, F. Haas, A. Hachem, G. A. Monnehan, A. Morsad, and M. Youlal

Centre de Recherches Nucléaires and Université Louis Pasteur, 67037 Strasbourg Cedex, France

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Vol. 38, Iss. 2 — August 1988

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