Zhu, L., Pillepich, A., Ven, G. v. d., Leaman, R., Hernquist, L., Nelson, D., . . . Zhang, L. (2022). Mass of the dynamically hot inner stellar halo predicts the ancient accreted stellar mass. Astronomy and astrophysics, 660, . https://doi.org/10.1051/0004-6361/202142496
Chicago Style (17th ed.) CitationZhu, Ling, Annalisa Pillepich, Glenn van de Ven, Ryan Leaman, Lars Hernquist, Dylan Nelson, Rüdiger Pakmor, Mark Vogelsberger, and Le Zhang. "Mass of the Dynamically Hot Inner Stellar Halo Predicts the Ancient Accreted Stellar Mass." Astronomy and Astrophysics 660 (2022). https://doi.org/10.1051/0004-6361/202142496.
MLA (9th ed.) CitationZhu, Ling, et al. "Mass of the Dynamically Hot Inner Stellar Halo Predicts the Ancient Accreted Stellar Mass." Astronomy and Astrophysics, vol. 660, 2022, https://doi.org/10.1051/0004-6361/202142496.