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102. 19Ne levels studied with the18F(d,n)19Ne*(18F+p) reaction

103. Single-nucleon transfer reactions on18F

104. First proton-transfer study of18F+presonances relevant for novae

106. Determination of theE1component of the low-energyC12(α,γ)O16cross section

107. AZURE: AnR-matrix code for nuclear astrophysics

110. Nuclear excitations at constant temperature

114. The S[sub E1] factor of the [sup 12]C(α,γ)[sup 16]O Reaction and the [sup 16]N β-delayed α Decay

117. New Determination of the AstrophysicalSFactorSE1of theC12(α,γ)O16Reaction

118. Measurement of the Cascade Transition via the First Excited State ofO16in theC12(α,γ)O16Reaction, and ItsSFactor in Stellar Helium Burning

119. Astrophysically importantSi26states studied with theSi28(p,t)Si26reaction. II. Spin of the 5.914-MeVSi26level and galacticAl26production

120. Proton-He3elastic scattering at low energies

121. Level density ofFe56and low-energy enhancement of γ-strength function

123. Neutron single particle strengths from the (d,p) reaction onF18

125. Elastic scattering of the proton drip-line nucleusF17

128. New constraints on theF18(p,α)O15rate in novae from the(d,p)reaction

131. Recent experimental results on level densities for compound reaction calculations.

133. Multistep processes in the12C(6Li,d)stripping reaction

134. Level Densities of Residual Nuclei from particle evaporation of 64Cu.

135. The SE1 factor of the 12C(α,γ)16O Reaction and the 16N β-delayed α Decay.

136. Kyy′(0°)for3He(d,p)4Henear theJπ=32+resonance

138. Level densities of iron isotopes and low-energy enhancement of γ-strength function.

140. THE SINGLE-PARTICLE STRUCTURE OF NEUTRON-RICH NUCLEI OF ASTROPHYSICAL INTEREST AT THE ORNL HRIBF.

143. Destruction of18Fvia18F(p,α)15Oburning through theEc.m.=665keV resonance

144. Proton-deuteron elastic scattering at low energies

146. Sub-Coulomb alpha transfer reactions.

147. The astrophysically important3+state in18Neand the17F(p,γ)18Nestellar rate

148. Kinematically complete measurement of the1H(18F,p)18Fexcitation function for the astrophysically important 7.08-MeV state in19Ne

150. Determination of the asymptoticD- toS-state ratio for6Livia(6Li→,d)transfer reactions

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