van Sluijs, L., Birkby, J. L., Lothringer, J., Lee, E. K. H., Crossfield, I. J. M., Parmentier, V., . . . Charbonneau, D. (2023). Carbon monoxide emission lines reveal an inverted atmosphere in the ultra hot Jupiter WASP-33 b consistent with an eastward hot spot. Monthly Notices of the Royal Astronomical Society, 522(2), 2145. https://doi.org/10.1093/mnras/stad1103
Chicago Style (17th ed.) Citationvan Sluijs, Lennart, et al. "Carbon Monoxide Emission Lines Reveal an Inverted Atmosphere in the Ultra Hot Jupiter WASP-33 B Consistent with an Eastward Hot Spot." Monthly Notices of the Royal Astronomical Society 522, no. 2 (2023): 2145. https://doi.org/10.1093/mnras/stad1103.
MLA (9th ed.) Citationvan Sluijs, Lennart, et al. "Carbon Monoxide Emission Lines Reveal an Inverted Atmosphere in the Ultra Hot Jupiter WASP-33 B Consistent with an Eastward Hot Spot." Monthly Notices of the Royal Astronomical Society, vol. 522, no. 2, 2023, p. 2145, https://doi.org/10.1093/mnras/stad1103.