Hansen, C. J., Andersen, A. C., & Christlieb, N. (2014). Stellar abundances and presolar grains trace the nucleosynthetic origin of molybdenum and ruthenium. Astronomy and astrophysics, 568, . https://doi.org/10.1051/0004-6361/201423535
Chicago Style (17th ed.) CitationHansen, Camilla Juul, Anja C. Andersen, and Norbert Christlieb. "Stellar Abundances and Presolar Grains Trace the Nucleosynthetic Origin of Molybdenum and Ruthenium." Astronomy and Astrophysics 568 (2014). https://doi.org/10.1051/0004-6361/201423535.
MLA (9th ed.) CitationHansen, Camilla Juul, et al. "Stellar Abundances and Presolar Grains Trace the Nucleosynthetic Origin of Molybdenum and Ruthenium." Astronomy and Astrophysics, vol. 568, 2014, https://doi.org/10.1051/0004-6361/201423535.
Warning: These citations may not always be 100% accurate.