Cite
Potential PeVatron supernova remnant G106.3+2.7 seen in the highest-energy gamma rays.
MLA
The Tibet ASγ Collaboration, et al. “Potential PeVatron Supernova Remnant G106.3+2.7 Seen in the Highest-Energy Gamma Rays.” Nature Astronomy, vol. 5, no. 5, May 2021, pp. 460–64. EBSCOhost, https://doi.org/10.1038/s41550-020-01294-9.
APA
The Tibet ASγ Collaboration, Amenomori, M., Bao, Y. W., Bi, X. J., Chen, D., Chen, T. L., Chen, W. Y., Chen, X., Chen, Y., Cirennima, Cui, S. W., Danzengluobu, Ding, L. K., Fang, J. H., Fang, K., Feng, C. F., Feng, Z., Feng, Z. Y., Gao, Q., & Gou, Q. B. (2021). Potential PeVatron supernova remnant G106.3+2.7 seen in the highest-energy gamma rays. Nature Astronomy, 5(5), 460–464. https://doi.org/10.1038/s41550-020-01294-9
Chicago
The Tibet ASγ Collaboration, M. Amenomori, Y. W. Bao, X. J. Bi, D. Chen, T. L. Chen, W. Y. Chen, et al. 2021. “Potential PeVatron Supernova Remnant G106.3+2.7 Seen in the Highest-Energy Gamma Rays.” Nature Astronomy 5 (5): 460–64. doi:10.1038/s41550-020-01294-9.