JINA - Virtual Journal of Nuclear Astrophysics, 5 April 2019
Volume 17, Issue 14 (22 Articles)
- # 1 - A Constant LGRB Metallicity Distribution Across Redshifts z < 2.5. (arXiv:1904.02673v1 [astro-ph.HE])
- # 2 - A metal-poor ultra compact dwarf galaxy at a kiloparsec distance from the low-mass elliptical galaxy FCC47. (arXiv:1904.01041v1 [astro-ph.GA])
- # 3 - An old, metal-poor globular cluster in Sextans A and the metallicity floor of globular cluster systems. (arXiv:1904.01084v1 [astro-ph.GA])
- # 4 - Constraining the properties of neutron-star matter with observations. (arXiv:1904.01354v1 [astro-ph.HE])
- # 5 - Determination of the primordial helium abundance based on NGC 346 an HII region of the Small Magellanic Cloud. (arXiv:1904.01594v1 [astro-ph.GA])
- # 6 - Extremely metal-poor galaxies with HST/COS: laboratories for models of low-metallicity massive stars and high-redshift galaxies. (arXiv:1904.01615v1 [astro-ph.GA])
- # 7 - Magnetorotational Mechanism of the Explosion of Core-Collapse Supernovae. (arXiv:1903.12628v1 [astro-ph.HE])
- # 8 - Metallicity and ionization state of the gas in polar-ring galaxies. (arXiv:1904.02513v1 [astro-ph.GA])
- # 9 - Nucleosynthesis in advective disc and outflow: possible explanation for overabundances in winds from X-ray binaries. (arXiv:1904.01592v1 [astro-ph.HE])
- # 10 - The origin of stellar populations in the Galactic bulge from chemical abundances. (arXiv:1903.12440v1 [astro-ph.GA])
- # 11 - Thermonuclear (Type Ia) Supernovae and Progenitor Evolution. (arXiv:1904.02238v1 [astro-ph.SR])
- # 12 - Ultra-heavy cosmic-ray science--Are r-process nuclei in the cosmic rays produced in supernovae or binary neutron star mergers?. (arXiv:1903.12228v1 [astro-ph.HE])
- # 13 - $beta$ and $beta$-delayed neutron decay of the $N=82$ nucleus $^{131}_{~49}$In$_{82}$. (arXiv:1903.12277v1 [nucl-ex])
- # 14 - Importance of $alpha$-induced reactions and the inverse $(gamma,alpha)$ on $p$-nuclei. (arXiv:1904.01809v1 [nucl-th])
- # 15 - Neutron skins as laboratory constraints on properties of neutron stars and what we can learn from heavy ion fragmentation reactions. (arXiv:1904.01078v1 [nucl-th])
- # 16 - Gamma-Ray Emission During the Accretion of Matter from a Supernova Envelope onto a Compact Remnant
- # 17 - Gravitational-wave hunt restarts — with a quantum boost
- Gravitational-wave hunt restarts — with a quantum boost
- https://www.nature.com/articles/d41586-019-01064-2
- # 18 - Optimization of lithium-glass fibers with lithium depleted coating for neutron detection
- # 19 - Precision measurement of the angular distribution for the 16O(d, p)17O transfer reaction to the ground state of 17O
- # 20 - Consistent relativistic mean-field models constrained by GW170817
- Physical Review C
- http://link.aps.org/doi/10.1103/PhysRevC.99.045202
- # 21 - The Helium Abundance of NGC 6791 from Modeling of Stellar Oscillations
- The Astrophysical Journal
- http://iopscience.iop.org/0004-637X/874/2/180
- # 22 - The R -Process Alliance: Discovery of a Low- α , r -process-enhanced Metal-poor Star in the Galactic
Halo
- The Astrophysical Journal
- http://iopscience.iop.org/0004-637X/874/2/148