no code implementations • 9 Feb 2021 • Fiorenzo Vincenzo, Todd A. Thompson, David H. Weinberg, Emily J. Griffith, James W. Johnson, Jennifer A. Johnson
We test the hypothesis that the observed first-peak (Sr, Y, Zr) and second-peak (Ba) s-process elemental abundances in low-metallicity Milky Way stars, and the abundances of the elements Mo and Ru, can be explained by a pervasive r-process contribution originating in neutrino-driven winds from highly-magnetic and rapidly rotating proto-neutron stars (proto-NSs).
Astrophysics of Galaxies High Energy Astrophysical Phenomena Solar and Stellar Astrophysics
1 code implementation • 19 Sep 2018 • T. Jayasinghe, K. Z. Stanek, C. S. Kochanek, B. J. Shappee, T. W. -S. Holoien, Todd A. Thompson, J. L. Prieto, Subo Dong, M. Pawlak, O. Pejcha, J. V. Shields, G. Pojmanski, S. Otero, C. A. Britt, D. Will
The variable stars in the VSX catalog are derived from a multitude of inhomogeneous data sources and classification tools.
Solar and Stellar Astrophysics
