Abundances of neutron-capture elements in CH and carbon-enhanced metal-poor (CEMP) stars
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DOI: 10.1007/s12036-020-09656-5
Abstract: All the elements heavier than Fe are produced either by the slow (-s) or rapid (-r) neutron-capture process. The neutron density prevailing in the stellar sites is one of the major factors that determines the… read more here.
Keywords: carbon; capture elements; neutron capture; cemp stars ... See more keywords