– Niels Bohr Institute - University of Copenhagen

Stellar abundances and presolar grains trace the nucleosynthetic origin of molybdenum and ruthenium

Research output: Contribution to journalJournal articleResearchpeer-review

C. J. Hansen, A. C. Andersen, N. Christlieb

Original languageEnglish
Article numberA47
JournalAstronomy & Astrophysics
Volume568
Number of pages17
ISSN0004-6361
DOIs
Publication statusPublished - 4 Aug 2014

    Research areas

  • stars: abundances, stars: general, meteorites, meteors, meteoroids, Galaxy: evolution, solar neighborhood

ID: 131403582