The Gaia BH3 companion exhibits an r-I abundance pattern reproduced by core-collapse supernova plus r-process yields and closely matching diluted ED-2 stars, supporting early cluster enrichment over local pollution.
year = 2003, month = sep, volume =
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A more efficient 12C+12C rate extends carbon burning, produces less compact pre-supernova structures, and enhances s-process yields of elements heavier than Fe in supernova ejecta from 15-40 solar mass stars.
Independent half-life determinations for 110Sn (4.165(25) h), 113Sn (116.08(94) d), 117mSn (13.95(1) d), and 123mSn (39.95(12) min) show general agreement with prior evaluations except for a clear discrepancy in 117mSn.
citing papers explorer
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The chemical fingerprint of the Gaia BH3 system. Evidence for early cluster enrichment from the analysis of 51 elements
The Gaia BH3 companion exhibits an r-I abundance pattern reproduced by core-collapse supernova plus r-process yields and closely matching diluted ED-2 stars, supporting early cluster enrichment over local pollution.
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Impact of Sub-2.5 MeV 12C+12CResonances on the Production of Elements from C to Pd in Core-Collapse Supernovae
A more efficient 12C+12C rate extends carbon burning, produces less compact pre-supernova structures, and enhances s-process yields of elements heavier than Fe in supernova ejecta from 15-40 solar mass stars.
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Half-Life Measurements of $^{110}$Sn, $^{113}$Sn, $^{117\mathrm{m}}$Sn, and $^{123\mathrm{m}}$Sn Produced via Photon Activation of Natural Tin
Independent half-life determinations for 110Sn (4.165(25) h), 113Sn (116.08(94) d), 117mSn (13.95(1) d), and 123mSn (39.95(12) min) show general agreement with prior evaluations except for a clear discrepancy in 117mSn.