Hirano, S., Sakai, Y., & Umeda, H. (2026). Formation of first star clusters under the supersonic gas flow – III. Environmental trends and halo-to-halo scatter in the Pop III IMF. Monthly Notices of the Royal Astronomical Society, 548(3), 1. https://doi.org/10.1093/mnras/stag634
Chicago Style (17th ed.) CitationHirano, Shingo, Yusuke Sakai, and Hideyuki Umeda. "Formation of First Star Clusters Under the Supersonic Gas Flow – III. Environmental Trends and Halo-to-halo Scatter in the Pop III IMF." Monthly Notices of the Royal Astronomical Society 548, no. 3 (2026): 1. https://doi.org/10.1093/mnras/stag634.
MLA (9th ed.) CitationHirano, Shingo, et al. "Formation of First Star Clusters Under the Supersonic Gas Flow – III. Environmental Trends and Halo-to-halo Scatter in the Pop III IMF." Monthly Notices of the Royal Astronomical Society, vol. 548, no. 3, 2026, p. 1, https://doi.org/10.1093/mnras/stag634.