Cite
Persistent Non-Gaussian Structure in the Image of Sagittarius A* at 86 GHz.
MLA
Issaoun, S., et al. “Persistent Non-Gaussian Structure in the Image of Sagittarius A* at 86 GHz.” Astrophysical Journal, vol. 915, no. 2, July 2021, pp. 1–14. EBSCOhost, https://doi.org/10.3847/1538-4357/ac00b0.
APA
Issaoun, S., Johnson, M. D., Blackburn, L., Broderick, A., Tiede, P., Wielgus, M., Doeleman, S. S., Falcke, H., Akiyama, K., Bower, G. C., Brinkerink, C. D., Chael, A., Cho, I., Gómez, J. L., Hernández-Gómez, A., Hughes, D., Kino, M., Krichbaum, T. P., Liuzzo, E., & Loinard, L. (2021). Persistent Non-Gaussian Structure in the Image of Sagittarius A* at 86 GHz. Astrophysical Journal, 915(2), 1–14. https://doi.org/10.3847/1538-4357/ac00b0
Chicago
Issaoun, S., M. D. Johnson, L. Blackburn, A. Broderick, P. Tiede, M. Wielgus, S. S. Doeleman, et al. 2021. “Persistent Non-Gaussian Structure in the Image of Sagittarius A* at 86 GHz.” Astrophysical Journal 915 (2): 1–14. doi:10.3847/1538-4357/ac00b0.