JINA - Virtual Journal of Nuclear Astrophysics, 18 May 2018
Volume 16, Issue 20 (19 Articles)
- # 1 - $s$-Process in Massive Carbon-Enhanced Metal-Poor Stars. (arXiv:1805.04306v1 [astro-ph.SR])
- # 2 - Chemical abundances of hydrostatic and explosive alpha-elements in Sagittarius stream stars. (arXiv:1805.04120v1 [astro-ph.GA])
- # 3 - Consistent Modeling of GS 1826-24 X-ray Bursts for Multiple Accretion Rates Demonstrates the Possibility to Constrain rp-process Reaction Rates. (arXiv:1805.05552v1 [astro-ph.HE])
- # 4 - Effects of thermonuclear X-ray bursts on non-burst emissions in the soft state of 4U 1728--34. (arXiv:1805.05393v1 [astro-ph.HE])
- # 5 - Gamma-Ray Astrophysics. (arXiv:1805.05642v1 [astro-ph.HE])
- # 6 - On the Red Giant Branch: Ambiguity in the Surface Boundary Condition Leads to ~100 K Uncertainty in Model Effective Temperatures. (arXiv:1805.04112v1 [astro-ph.SR])
- # 7 - Possible white dwarf progenitors of type Ia supernovae. (arXiv:1805.04845v1 [astro-ph.SR])
- # 8 - r-Process Nucleosynthesis: Connecting Rare-Isotope Beam Facilities with the Cosmos. (arXiv:1805.04637v1 [astro-ph.SR])
- # 9 - Should Type Ia Supernova Distances be Corrected for their Local Environments?. (arXiv:1805.05911v1 [astro-ph.CO])
- # 10 - Study of the abundance features of the metal-poor star HD 94028. (arXiv:1805.04235v1 [astro-ph.SR])
- # 11 - The beginning of nonlinear stage of evolution of protostars at $ z=20. (arXiv:1805.04430v1 [astro-ph.CO])
- # 12 - The lowest metallicity type II supernova from the highest mass red-supergiant progenitor. (arXiv:1805.04434v1 [astro-ph.HE])
- # 13 - The Smoking Guns Of Neutron Stars Mergers. (arXiv:1805.06319v1 [astro-ph.HE])
- # 14 - X-ray Absorption in Young Core-Collapse Supernova Remnants. (arXiv:1805.04528v1 [astro-ph.HE])
- # 15 - Nuclear Astrophysics in the New Era of Multimessenger Astronomy. (arXiv:1805.04780v1 [nucl-th])
- # 16 - The evolution of the X-ray afterglow emission of GW 170817/ GRB 170817A in XMM-Newton observations
- Astronomy & Astrophysics
- http://feedproxy.google.com/~r/edp_aa/~3/BewHh2J_LsM/201832664
- # 17 - Characterizing the astrophysical $S$ factor for $^{12}mathrm{C}+^{12}mathrm{C}$ fusion with wave-packet dynamics
- Physical Review C
- http://link.aps.org/doi/10.1103/PhysRevC.97.055802
- # 18 - Neutron stars' quark matter not so strange
- # 19 - An Empirical Fitting Method to Type Ia Supernova Light Curves. III. A Three-parameter Relationship:
Peak Magnitude, Rise Time, and Photospheric Velocity
- The Astrophysical Journal
- http://iopscience.iop.org/0004-637X/858/2/104