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Autor:
Cameron Angus, Matthew Williams, Andrei Andreyev, Soumendu Bhattacharjee, Samantha Buck, Soham Chakraborty, Barry Davids, Christian Diget, Adam Garnsworthy, Chris Griffin, Asunción Fernandez, Greg Hackman, Kevan Hudson, Dirk Hufschmidt, Vasil Karayonchev, Yong Kim, Alison Laird, Annika Lennarz, Konstantin Mashtakov, Peter Machule, Connor Natzke, Kihong Pak, Athanasios Psaltis, Allison Radich, Thomas Rauscher, Daniel Rhodes, Thierry Sauvage, Anna Simon, Carl Svensson, Sriteja Upadhyayula, Jonathan Williams, Daniel Yates, Tammy Zidar
Publikováno v:
EPJ Web of Conferences. 279:11003
The r-process has been shown to be robust in reproducing the abundance distributions of heavy elements, such as europium, seen in ultra-metal poor stars. In contrast, observations of elements 26 < Z < 47 display overabundances relative to r-process m
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::4411d053c748709ea4c7c465dcb88f6e
https://doi.org/10.1051/epjconf/202327911003
https://doi.org/10.1051/epjconf/202327911003
