Jansen, C. A.; Burkhardt, C.; Marrocchi, Y.; Schneider, J. M.; Wölfer, E.; Kleine, T.: Condensate evolution in the solar nebula inferred from combined Cr, Ti, and O isotope analyses of amoeboid olivine aggregates. Earth and Planetary Science Letters 627, p. 118567 (2024)
Jansen, C. A.; Burkhardt, C.; Marrocchi, Y.; Schneider, J.M.; Wölfer, E.; Kleine, T.: Condensate evolution in the solar nebula inferred from combined Cr, Ti, and O isotope analyses of amoeboid olivine aggregates. Earth and Planetary Science Letters 627, p. 118567 (2024)
Schneider, J.M.; Kleine, T.: Effects of Faraday cup deterioration on Sr and Cr isotope analyses by thermal ionization mass spectrometry. JOURNAL OF ANALYTICAL ATOMIC SPECTROMETRY (7), pp. 1910 - 1918 (2024)
Schneider, J. M.; Burkhardt, C.; Kleine, T.: Distribution of s-, r-, and p-process Nuclides in the Early Solar System Inferred from Sr Isotope Anomalies in Meteorites. The Astrophysical Journal 952, p. L25 (2023)
Windmill, R. J.; Franchi, I. A.; Hellmann, J. L.; Schneider, J. M.; Fridolin, S.; Kleine, T.; Greenwood, R. C.; Anand, M.: Isotopic evidence for pallasite formation by impact mixing of olivine and metal during the first 10 million years of the Solar System. PNAS Nexus 1 (1) (2022)
A star’s chemical composition strongly influences the ultraviolet radiation it emits into space and thus the conditions for the emergence of life in its neighbourhood.
A single star has provided information about the collision of the Milky Way with the dwarf galaxy Gaia-Enceladus. The event likely took place approximately 11.5 billion years ago.