The level structure of 20Na and the impact upon the stellar reaction rate for 19Ne(p, γ)20Na
- 1 April 1990
- journal article
- Published by Elsevier in Nuclear Physics A
- Vol. 510 (3) , 503-517
- https://doi.org/10.1016/0375-9474(90)90063-r
Abstract
No abstract availableKeywords
This publication has 21 references indexed in Scilit:
- A modified position sensitive proportional counter with improved particle identification capabilityNuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, 1989
- Energy levels of light nuclei A = 18–20Nuclear Physics A, 1987
- Measurement of the 15N(α, γ)19F resonances at Ec.m. = 536 keV and 542 keVNuclear Physics A, 1987
- A new estimate of the Ne-19(p, gamma) Na-20 and O-15(alpha, gamma) Ne-19 reaction rates at stellar energiesThe Astrophysical Journal, 1986
- Energy levels of light nuclei A = 18–20Nuclear Physics A, 1983
- Explosive hydrogen burningThe Astrophysical Journal Supplement Series, 1981
- Energy levels of light nuclei A = 18–20Nuclear Physics A, 1978
- Hot CNO-Ne Cycle Hydrogen Burning. Thermonuclear Evolution at Constant Temperature and DensityThe Astrophysical Journal, 1973
- Design and performance of a new magnetic spectrograph for accurate energy measurementsNuclear Instruments and Methods, 1973
- Calculation of the G factor for gas scattering experimentsNuclear Instruments and Methods, 1959