JINA - Virtual Journal of Nuclear Astrophysics, 7 February 2020
Volume 18, Issue 6 (15 Articles)
- # 1 - Can Kilonova Light curves be Standardized?. (arXiv:1908.02168v2 [astro-ph.SR] UPDATED)
- # 2 - High-energy Cosmic Ray production in X-ray Binary Jets. (arXiv:2002.01477v1 [astro-ph.HE])
- # 3 - Observational and theoretical constraints on the formation and early evolution of the first dust grains in galaxies at 5 < z < 10. (arXiv:2002.01858v1 [astro-ph.GA])
- # 4 - SNe Ia from double detonations: Impact of core-shell mixing on the carbon ignition mechanism. (arXiv:2002.00981v1 [astro-ph.SR])
- # 5 - Stripped-envelope core-collapse supernova $^{56}$Ni masses: Persistently larger values than supernovae type II. (arXiv:2002.01015v1 [astro-ph.HE])
- # 6 - Supernova Siblings: Assessing the Consistency of Properties of Type Ia Supernovae that Share the Same Parent Galaxies. (arXiv:2002.00974v1 [astro-ph.GA])
- # 7 - The origin of s-process isotope heterogeneity in the solar protoplanetary disk. (arXiv:2002.02155v1 [astro-ph.EP])
- # 8 - Constraining the destruction rate of 40K in stellar nucleosynthesis through the study of the 40Ar(p,n)40K reaction. (arXiv:2001.11600v1 [nucl-ex])
- # 9 - The -ball -spectrometer
- # 10 - Asymptotic normalization coefficients from transfer reactions and $R$-matrix analysis of direct capture in the $^{22}mathrm{Ne}(p,γ)^{23}mathrm{Na}$ reaction
- Physical Review C
- http://link.aps.org/doi/10.1103/PhysRevC.101.025802
- # 11 - Measurement of $^{34}mathrm{S}(^{3}mathrm{He},p)^{36}mathrm{Cl}$ cross sections for nuclide enrichment in the early solar system
- Physical Review C
- http://link.aps.org/doi/10.1103/PhysRevC.101.025801
- # 12 - Decay properties of 22Ne + α resonances and their impact on s-process nucleosynthesis
- # 13 - Astronuclear Physics: A tale of the atomic nuclei in the skies
- # 14 - Gamma Rays from Kilonova: A Potential Probe of r -process Nucleosynthesis
- The Astrophysical Journal
- http://iopscience.iop.org/0004-637X/889/2/168
- # 15 - Study of the $${{^{25}}}$$25 Mg(d,p) $${{^{26}}}$$26 Mg reaction to constrain the $${{^{25}}}$$25 Al(p, $${gamma }$$γ ) $${{^{26}}}$$26 Si resonant reaction rates in nova burning conditions