Observation of the 190 keV Resonance in ^17O(p,γ)^18F

Details Observation of the 190 keV Resonance in ^17O(p,γ)^18F Observation of the 190 keV Resonance in ^17O(p,γ)^18F

May 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aps..apr.j8009f&link_type=abstract

American Physical Society, April Meeting, 2004, May 1-4, 2004, Denver, Colorado April 2004, MEETING ID: APR04, abstract #J8.009

Astronomy and Astrophysics

Astrophysics

Scientific paper

The ^17O(p,γ)^18F reaction influences the production of the stable isotope ^17O and of the radionuclide ^18F in nova bursts. The current reaction rate uncertainty amounts to several orders of magnitude at the important stellar temperatures and is caused by a previously unobserved resonance at ˜ 180 keV. We report on the first direct observation of this particular resonance. Our preliminary findings yield a resonance strength of ωγ ˜ 2x10-6 eV. A discussion of the astrophysical implications will be presented.

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