Hydrogen Burning of $^{17}$O in Classical Novae
dc.contributor.author | CHAFA, A. | |
hal.structure.identifier | Centre de Spectrométrie Nucléaire et de Spectrométrie de Masse [CSNSM] | |
dc.contributor.author | TATISCHEFF, V. | |
hal.structure.identifier | Centre d'Etudes Nucléaires de Bordeaux Gradignan [CENBG] | |
dc.contributor.author | AGUER, P. | |
dc.contributor.author | BARHOUMI, S. | |
hal.structure.identifier | Centre de Spectrométrie Nucléaire et de Spectrométrie de Masse [CSNSM] | |
dc.contributor.author | COC, A. | |
hal.structure.identifier | Centre de Spectrométrie Nucléaire et de Spectrométrie de Masse [CSNSM] | |
dc.contributor.author | GARRIDO, F. | |
dc.contributor.author | HERNANZ, M. | |
dc.contributor.author | JOSE, J. | |
hal.structure.identifier | Centre de Spectrométrie Nucléaire et de Spectrométrie de Masse [CSNSM] | |
dc.contributor.author | KIENER, J. | |
hal.structure.identifier | Centre de Spectrométrie Nucléaire et de Spectrométrie de Masse [CSNSM] | |
dc.contributor.author | LEFEBVRE-SCHUHL, A. | |
dc.contributor.author | OUICHAOUI, S. | |
hal.structure.identifier | Centre de Spectrométrie Nucléaire et de Spectrométrie de Masse [CSNSM] | |
dc.contributor.author | DE SEREVILLE, N. | |
hal.structure.identifier | Centre de Spectrométrie Nucléaire et de Spectrométrie de Masse [CSNSM] | |
dc.contributor.author | THIBAUD, J. -P. | |
dc.date.created | 2005 | |
dc.date.issued | 2005 | |
dc.identifier.issn | 0031-9007 | |
dc.description.abstractEn | We report on the observation of a previously unknown resonance at E=194.1+/-0.6 keV (lab) in the 17-O(p,alpha)14-N reaction, with a measured resonance strength omega_gamma(p,alpha)=1.6+/-0.2 meV. We studied in the same experiment the 17-O(p,gamma)18-F reaction by an activation method and the resonance-strength ratio was found to be omega_gamma(p,alpha)/omega_gamma(p,gamma)=470+/-50. The corresponding excitation energy in the 18-F compound nucleus was determined to be 5789.8+/-0.3 keV by gamma-ray measurements using the 14-N(alpha,gamma)18-F reaction. These new resonance properties have important consequences for 17-O nucleosynthesis and gamma-ray astronomy of classical novae. | |
dc.language.iso | en | |
dc.publisher | American Physical Society | |
dc.subject.en | proton-nucleus reactions | |
dc.subject.en | proton radiative capture | |
dc.subject.en | alpha particle-nucleus reactions | |
dc.subject.en | novae | |
dc.subject.en | nuclear energy level transitions | |
dc.subject.en | nucleosynthesis | |
dc.title.en | Hydrogen Burning of $^{17}$O in Classical Novae | |
dc.type | Article de revue | |
dc.identifier.doi | 10.1103/PhysRevLett.95.031101 | |
dc.subject.hal | Physique [physics]/Astrophysique [astro-ph]/Cosmologie et astrophysique extra-galactique [astro-ph.CO] | |
dc.subject.hal | Physique [physics]/Physique Nucléaire Expérimentale [nucl-ex] | |
dc.subject.hal | Planète et Univers [physics]/Astrophysique [astro-ph] | |
dc.identifier.arxiv | astro-ph/0506500 | |
bordeaux.journal | Physical Review Letters | |
bordeaux.page | 031101 (4 pages) | |
bordeaux.volume | 95 | |
bordeaux.peerReviewed | oui | |
hal.identifier | in2p3-00024492 | |
hal.version | 1 | |
hal.popular | non | |
hal.audience | Non spécifiée | |
hal.origin.link | https://hal.archives-ouvertes.fr//in2p3-00024492v1 | |
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