JINA - Virtual Journal of Nuclear Astrophysics, 8 January 2016
Volume 14, Issue 2 (23 Articles)
- # 1 - A new neutrino source for the study of the solar neutrino physics in the vacuum-matter transition region
- arXiv.org - Astrophysics - Volume: 2016, Issue: 8 Jan
- arXiv:1601.00377 [pdf, ps, other]
- # 2 - A prevalence of dynamo-generated magnetic fields in the cores of intermediate-mass stars
- arXiv.org - Astrophysics - Volume: 2016, Issue: 8 Jan
- arXiv:1601.00004 [pdf, other]
- # 3 - An Intermediate Type Ia Supernova Between Normal And Super-Chandrasekhar
- arXiv.org - Astrophysics - Volume: 2016, Issue: 8 Jan
- arXiv:1601.00686 [pdf, other]
- # 4 - Chemodynamic subpopulations of the Carina dwarf galaxy
- arXiv.org - Astrophysics - Volume: 2016, Issue: 8 Jan
- arXiv:1601.01589 [pdf, other]
- # 5 - How plausible are the proposed formation scenarios of CEMP-r/s stars?
- arXiv.org - Astrophysics - Volume: 2016, Issue: 8 Jan
- arXiv:1601.00976 [pdf, other]
- # 6 - Light Sterile Neutrinos In Cosmology
- arXiv.org - Astrophysics - Volume: 2016, Issue: 8 Jan
- arXiv:1601.01475 [pdf, other]
- # 7 - Linking 1D Evolutionary to 3D Hydrodynamical Simulations of Massive Stars
- arXiv.org - Astrophysics - Volume: 2016, Issue: 8 Jan
- arXiv:1601.01572 [pdf, other]
- # 8 - Milky Way chemo-dynamics in the era of Gaia
- arXiv.org - Astrophysics - Volume: 2016, Issue: 8 Jan
- arXiv:1601.01313 [pdf, ps, other]
- # 9 - On Potassium and Other Abundance Anomalies of Red Giants in NGC 2419
- arXiv.org - Astrophysics - Volume: 2016, Issue: 8 Jan
- arXiv:1601.01359 [pdf, other]
- # 10 - On the Diversity of Compact Objects within Supernova Remnants. I: A Parametric Model for Magnetic Field Evolution
- arXiv.org - Astrophysics - Volume: 2016, Issue: 8 Jan
- arXiv:1601.00949 [pdf, ps, other]
- # 11 - Progenitor constraints for core-collapse supernovae from Chandra X-ray observations
- arXiv.org - Astrophysics - Volume: 2016, Issue: 8 Jan
- arXiv:1601.00871 [pdf, ps, other]
- # 12 - Rapid rotational crust-core relaxation in magnetars
- arXiv.org - Astrophysics - Volume: 2016, Issue: 8 Jan
- arXiv:1601.00056 [pdf, ps, other]
- # 13 - The Unusual Super-Luminous Supernovae SN 2011kl and ASASSN-15lh
- arXiv.org - Astrophysics - Volume: 2016, Issue: 8 Jan
- arXiv:1601.01021 [pdf, ps, other]
- # 14 - Updated determination of the solar neutrino fluxes from solar neutrino data
- arXiv.org - Astrophysics - Volume: 2016, Issue: 8 Jan
- arXiv:1601.00972 (cross-list from hep-ph) [pdf, other]
- # 15 - Underground nuclear astrophysics: why and how
- arXiv.org - Nuclear Experiment - Volume: 2016, Issue: 8 Jan
- arXiv:1601.00188 [pdf, other]
- # 16 - Fractionized Skyrmions in Dense Compact-Star Matter
- arXiv.org - Nuclear Theory - Volume: 2016, Issue: 8 Jan
- arXiv:1601.00058 [pdf, ps, other]
- # 17 - Hyperons in neutron stars and supernova cores
- arXiv.org - Nuclear Theory - Volume: 2016, Issue: 8 Jan
- arXiv:1601.00435 [pdf, ps, other]
- # 18 - Microsopic nuclear level densities by the shell model Monte Carlo method
- arXiv.org - Nuclear Theory - Volume: 2016, Issue: 8 Jan
- arXiv:1601.00118 [pdf, ps, other]
- # 19 - Pairing in high-density neutron matter including short- and long-range correlations
- arXiv.org - Nuclear Theory - Volume: 2016, Issue: 8 Jan
- arXiv:1601.01600 [pdf, other]
- # 20 - The shell model Monte Carlo approach to level densities: recent developments and perspectives
- arXiv.org - Nuclear Theory - Volume: 2016, Issue: 8 Jan
- arXiv:1601.00107 [pdf, other]
- # 21 - New insights on the spin-up of a neutron star during core collapse
- Monthly Notices of the Royal Astronomical Society - Volume: 456, Issue: 1
- Abstract Full Text (HTML) Full Text (PDF) SUPPORTING INFORMATION
- # 22 - Spin paramagnetic deformation of a neutron star
- Monthly Notices of the Royal Astronomical Society - Volume: 456, Issue: 1
- Abstract Full Text (HTML) Full Text (PDF)
- # 23 - Stability of metal-rich very massive stars
- Monthly Notices of the Royal Astronomical Society - Volume: 456, Issue: 1
- Abstract Full Text (HTML) Full Text (PDF)
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.

