Present and future studies with DRAGON at ISAC

Details Present and future studies with DRAGON at ISAC Present and future studies with DRAGON at ISAC

Oct 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aps..dnp.de011c&link_type=abstract

American Physical Society, 2002 Fall Meeting of the Division of Nuclear , abstract #DE.011

Astronomy and Astrophysics

Astronomy

Scientific paper

The isotope ^22Na (T_1/2 2.6 years) in nova ejecta may serve as an important target for gamma-ray astronomy with orbiting telescopes. The ^21Na(p,γ)^22Mg reaction, in turn, is a key link in the production of ^22Na in nova nucleosynthesis. We present recent results from a measurement of the ^21Na(p,γ)^22Mg reaction rate, using radioactive ^21Na beams from ISAC and the DRAGON recoil separator. We also discuss future plans to measure with DRAGON other reactions of importance to stellar explosions, such as ^13N(p,γ)^14O, ^19Ne(p,γ)^20Na, and ^25Al(p,γ)^26Si, among others.

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