Cite
Potential PeVatron supernova remnant G106.3+2.7 seen in the highest-energy gamma rays
MLA
Amenomori, M., et al. Potential PeVatron Supernova Remnant G106.3+2.7 Seen in the Highest-Energy Gamma Rays. 2021. EBSCOhost, https://doi.org/10.1038/s41550-020-01294-9.
APA
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., … Zhou, X. X. (2021). Potential PeVatron supernova remnant G106.3+2.7 seen in the highest-energy gamma rays. https://doi.org/10.1038/s41550-020-01294-9
Chicago
Amenomori, M., Y. W. Bao, X. J. Bi, D. Chen, T. L. Chen, W. Y. Chen, Xu Chen, et al. 2021. “Potential PeVatron Supernova Remnant G106.3+2.7 Seen in the Highest-Energy Gamma Rays.” doi:10.1038/s41550-020-01294-9.