JINA - Virtual Journal of Nuclear Astrophysics, 14 January 2011
Volume 9, Issue 2 (22 Articles)
- # 1 - Chemically tagging the Hyades stream: Does it partly originate from the Hyades cluster?
- arXiv.org - Astrophysics - Volume: 2011, Issue: 14 Jan
- arXiv:1101.2583 [pdf, ps, other]
- # 2 - Differentially-rotating neutron star models with a parametrized rotation profile
- arXiv.org - Astrophysics - Volume: 2011, Issue: 14 Jan
- arXiv:1101.2664 [pdf, ps, other]
- # 3 - First stars XIII. Two extremely metal-poor RR Lyrae stars?
- arXiv.org - Astrophysics - Volume: 2011, Issue: 14 Jan
- arXiv:1101.2207 [pdf, ps, other]
- # 4 - Nucleosynthesis and gamma-ray lines
- arXiv.org - Astrophysics - Volume: 2011, Issue: 14 Jan
- arXiv:1101.2112 [pdf, ps, other]
- # 5 - Quiet Novae with Flat Maximum -- No Optically Thick Winds
- arXiv.org - Astrophysics - Volume: 2011, Issue: 14 Jan
- arXiv:1101.2554 [pdf, ps, other]
- # 6 - Refined Neutron-Star Mass Determinations for Six Eclipsing X-Ray Pulsar Binaries
- arXiv.org - Astrophysics - Volume: 2011, Issue: 14 Jan
- arXiv:1101.2465 [pdf, ps, other]
- # 7 - SGR 0418+5729: a low-magnetic-field magnetar
- arXiv.org - Astrophysics - Volume: 2011, Issue: 14 Jan
- arXiv:1101.2299 [pdf, ps, other]
- # 8 - Theoretical Evaluation of the Reaction Rates for 26Al(n,p)26Mg and 26Al(n,a)23Na
- arXiv.org - Astrophysics - Volume: 2011, Issue: 14 Jan
- arXiv:1101.2265 [pdf, ps, other]
- # 9 - Topics on Galactic Chemical Evolution
- arXiv.org - Astrophysics - Volume: 2011, Issue: 14 Jan
- arXiv:1101.2108 [pdf, ps, other]
- # 10 - [O/Fe] Estimates for Carbon-Enhanced Metal-Poor Stars from Near-IR Spectroscopy
- arXiv.org - Astrophysics - Volume: 2011, Issue: 14 Jan
- arXiv:1101.2260 [pdf, ps, other]
- # 11 - An Optical Readout TPC (O-TPC) for Studies in Nuclear Astrophysics With Gamma-Ray Beams at HIgS
- arXiv.org - Nuclear Experiment - Volume: 2011, Issue: 14 Jan
- arXiv:1101.1940 (cross-list from physics.ins-det) [pdf]
- # 12 - Symmetry energy from elliptic flow in 197Au + 197Au
- arXiv.org - Nuclear Experiment - Volume: 2011, Issue: 14 Jan
- arXiv:1101.2361 [pdf, ps, other]
- # 13 - Ab initio calculation of the Hoyle state
- arXiv.org - Nuclear Theory - Volume: 2011, Issue: 14 Jan
- arXiv:1101.2547 [pdf, ps, other]
- # 14 - Astrophysical $S$ factor for the ${}^{15}{rm N}(p,gamma){}^{16}{rm O}$ reaction from $R$-matrix analysis and asymptotic normalization coefficient for ${}^{16}{rm O} to {}^{15}{rm N} + p$. Is any fit acceptable?
- arXiv.org - Nuclear Theory - Volume: 2011, Issue: 14 Jan
- arXiv:1101.1924 (cross-list from nucl-ex) [pdf, other]
- # 15 - Low-momentum interactions with Brown-Rho-Ericson scalings and the density dependence of the nuclear symmetry energy
- arXiv.org - Nuclear Theory - Volume: 2011, Issue: 14 Jan
- arXiv:1101.1910 [pdf, ps, other]
- # 16 - Shell model study for neutron-rich sd-shell nuclei
- arXiv.org - Nuclear Theory - Volume: 2011, Issue: 14 Jan
- arXiv:1101.1571 [pdf, ps, other]
- # 17 - Spectroscopic calculations of the low-lying structure in exotic Os and W isotopes
- arXiv.org - Nuclear Theory - Volume: 2011, Issue: 14 Jan
- arXiv:1101.1699 [pdf, ps, other]
- # 18 - Stability beyond the neutron drip-line near the third peak of the r-process nucleosynthesis
- arXiv.org - Nuclear Theory - Volume: 2011, Issue: 14 Jan
- arXiv:1101.2287 [pdf, ps, other]
- # 19 - The maximum mass and radius of neutron stars and the nuclear symmetry energy
- arXiv.org - Nuclear Theory - Volume: 2011, Issue: 14 Jan
- arXiv:1101.1921 [pdf, other]
- # 20 - Three-body structure of low-lying 18Ne states
- arXiv.org - Nuclear Theory - Volume: 2011, Issue: 14 Jan
- arXiv:1101.2376 [pdf, ps, other]
- # 21 - Heavy Cluster Knockout Reaction 16O(12C,212C)4He and the Nature of the 12C-12C Interaction Potential
- Physical Review Letters - Volume: 106, Issue: 2
- 022501 [View PDF (2,118 kB)]
- # 22 - An Evolving Stellar Initial Mass Function and the Gamma-ray Burst Redshift Distribution
- The Astrophysical Journal Letters - Volume: 727, Issue: 2
- Abstract References Full text PDF (274 KB) View as HTML
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.

