JINA - Virtual Journal of Nuclear Astrophysics, 26 January 2007
Volume 5, Issue 4 (19 Articles)
- # 1 - Quark Stars: Features and Findings
- # 2 - Revised Primordial Helium Abundance Based on New Atomic Data
- # 3 - A new constraint for gamma-ray burst progenitor mass
- # 4 - Winds of Main-Sequence Stars: Observational Limits and a Path to Theoretical Prediction
- # 5 - The Latitude of Type I X-Ray Burst Ignition on Rapidly Rotating Neutron Stars
- # 6 - Cosmological neutrino mass detection: The best probe of neutrino lifetime
- # 7 - Dark Energy, A Cosmological Constant, and Type Ia Supernovae
- # 8 - Stellar Evolutionary Models: challenges from observations of stellar systems
- # 9 - Supernova neutrino observations: What can we learn?
- # 10 - Nuclear symmetry potential in the relativistic impulse approximation
- # 11 - Direct mass measurements beyond the proton drip-line
- # 12 - High-precision mass measurements of nickel, copper, and gallium isotopes and the purported shell closure at N=40
- # 13 - Constraining the Skyrme effective interactions and the neutron skin thickness of nuclei using isospin diffusion data from heavy ion collisions
- # 14 - Temperature effects on the nuclear symmetry energy and symmetry free energy with an isospin and momentum dependent interaction
- # 15 - Variational Calculation for the Equation of State of Nuclear Matter at Finite Temperatures
- # 16 - Are spectroscopic factors from transfer reactions consistent with asymptotic normalisation coefficients?
- # 17 - The relation between nuclear charge radii and other parameters characterizing the nuclear drops
- # 18 - A LARGE STELLAR EVOLUTION DATABASE FOR POPULATION SYNTHESIS STUDIES. III. INCLUSION OF THE FULL ASYMPTOTIC GIANT BRANCH PHASE AND WEB TOOLS FOR STELLAR POPULATION ANALYSES
- Astronomical Journal - Volume 133, Issue 2
- Abstract Full Text with Enhancements PDF (496 kB)
- # 19 - AMERICAN ASTRONOMICAL SOCIETY MEETING: Middle-Earth Denizens Mob the Milky Way
This material is based upon work supported in part by the U.S. Department of Energy, Office of Science, Office of Nuclear Physics, under Award Number DE-SC0026204.