Add to ORKGClassical novae are important contributors to the abundances of key isotopes, such as the radioactive 18F, whose observation by satellite missions could provide constraints on nucleosynthesis models in novae. The 17O(p,gamma)18F reaction plays a critical role in the synthesis of both oxygen and fluorine isotopes but its reaction rate is not well determined because of the lack of experimental data at energies relevant to novae explosions. In this study, the reaction cross section has been measured directly for the first time in a wide energy range Ecm 43 200 12 370 keV appropriate to hydrogen burning in classical novae. In addition, the E=183 keV resonance strength, =1.67\ub10.12 \u3bceV, has been measured with the highest precision to dat...
Background: The O17(p,γ)F18 reaction affects the production of key isotopes (e.g., F18 and O18) in t...
Background: The O17(p,γ)F18 reaction affects the production of key isotopes (e.g., F18 and O18) in t...
Classical novae are explained as thermonuclear explosions on the surface of white dwarf stars accre...
Classical novae are important contributors to the abundances of key isotopes, such as the radioactiv...
Classical novae are important contributors to the abundances of key isotopes, such as the radioactiv...
Classical novae are important contributors to the abundances of key isotopes, such as the radioactiv...
Classical novae are important contributors to the abundances of key isotopes, such as the radioactiv...
Classical novae are important contributors to the abundances of key isotopes, such as the radioactiv...
Classical novae are important contributors to the abundances of key isotopes, such as the radioactiv...
Classical novae are important contributors to the abundances of key isotopes, such as the radioactiv...
Classical novae are important contributors to the abundances of key isotopes, such as the radioactiv...
Background: The 17O(p,\u3b3 )18F reaction affects the production of key isotopes (e.g., 18F and 18O)...
Classical novae are explosive binary systems involving the accretion of hydrogen rich material from ...
Classical novae are explosive binary systems involving the accretion of hydrogen rich material from ...
Background: The O17(p,γ)F18 reaction affects the production of key isotopes (e.g., F18 and O18) in t...
Background: The O17(p,γ)F18 reaction affects the production of key isotopes (e.g., F18 and O18) in t...
Background: The O17(p,γ)F18 reaction affects the production of key isotopes (e.g., F18 and O18) in t...
Classical novae are explained as thermonuclear explosions on the surface of white dwarf stars accre...
Classical novae are important contributors to the abundances of key isotopes, such as the radioactiv...
Classical novae are important contributors to the abundances of key isotopes, such as the radioactiv...
Classical novae are important contributors to the abundances of key isotopes, such as the radioactiv...
Classical novae are important contributors to the abundances of key isotopes, such as the radioactiv...
Classical novae are important contributors to the abundances of key isotopes, such as the radioactiv...
Classical novae are important contributors to the abundances of key isotopes, such as the radioactiv...
Classical novae are important contributors to the abundances of key isotopes, such as the radioactiv...
Classical novae are important contributors to the abundances of key isotopes, such as the radioactiv...
Background: The 17O(p,\u3b3 )18F reaction affects the production of key isotopes (e.g., 18F and 18O)...
Classical novae are explosive binary systems involving the accretion of hydrogen rich material from ...
Classical novae are explosive binary systems involving the accretion of hydrogen rich material from ...
Background: The O17(p,γ)F18 reaction affects the production of key isotopes (e.g., F18 and O18) in t...
Background: The O17(p,γ)F18 reaction affects the production of key isotopes (e.g., F18 and O18) in t...
Background: The O17(p,γ)F18 reaction affects the production of key isotopes (e.g., F18 and O18) in t...
Classical novae are explained as thermonuclear explosions on the surface of white dwarf stars accre...