摘要:Isotopic ratios of heavy elements are a key signature of the nucleosynthesis processes in
stellar interiors. The contribution of successive generations of stars to the metal
enrichment of the Universe is imprinted on the evolution of isotopic ratios over time. We
investigate the isotopic ratios of carbon, nitrogen, oxygen, and sulfur through millimeter
molecular absorption lines arising in the z = 0.68 absorber toward the blazar B 0218+357. We
find that these ratios differ from those observed in the Galactic interstellar medium, but
are remarkably close to those in the only other source at intermediate redshift for which
isotopic ratios have been measured to date, the z = 0.89 absorber in front of
PKS 1830−211. The isotopic
ratios in these two absorbers should reflect enrichment mostly from massive stars, and
they are indeed close to the values observed toward local starburst galaxies. Our
measurements set constraints on nucleosynthesis and chemical evolution models.