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Autor:
Kobayashi, Chiaki, Mandel, Ilya, Belczynski, Krzysztof, Goriely, Stephane, Janka, Thomas H., Just, Oliver, Ruiter, Ashley J., Van Beveren, Dany, Kruckow, Matthias U., Briel, Max M., Eldridge, Jan J., Stanway, Elizabeth
Comparing Galactic chemical evolution models to the observed elemental abundances in the Milky Way, we show that neutron star mergers can be a leading r-process site only if at low metallicities such mergers have very short delay times and significan
Externí odkaz:
http://arxiv.org/abs/2211.04964
