Rapidly rotating Population III stellar models as a source of primary nitrogen.

MLA

Tsiatsiou, Sophie, et al. “Rapidly Rotating Population III Stellar Models as a Source of Primary Nitrogen.” Astronomy & Astrophysics / Astronomie et Astrophysique, vol. 687, July 2024, pp. 1–17. EBSCOhost, https://doi.org/10.1051/0004-6361/202449156.

APA

Tsiatsiou, S., Sibony, Y., Nandal, D., Sciarini, L., Hirai, Y., Ekström, S., Farrell, E., Murphy, L., Choplin, A., Hirschi, R., Chiappini, C., Liu, B., Bromm, V., Groh, J., & Meynet, G. (2024). Rapidly rotating Population III stellar models as a source of primary nitrogen. Astronomy & Astrophysics / Astronomie et Astrophysique, 687, 1–17. https://doi.org/10.1051/0004-6361/202449156

Chicago

Tsiatsiou, Sophie, Yves Sibony, Devesh Nandal, Luca Sciarini, Yutaka Hirai, Sylvia Ekström, Eoin Farrell, et al. 2024. “Rapidly Rotating Population III Stellar Models as a Source of Primary Nitrogen.” Astronomy & Astrophysics / Astronomie et Astrophysique 687 (July): 1–17. doi:10.1051/0004-6361/202449156.