Cite
The relationship between polycyclic aromatic hydrocarbon emission and far-infrared dust emission from NGC 2403 and M83.
MLA
Jones, A. G., et al. “The Relationship between Polycyclic Aromatic Hydrocarbon Emission and Far-Infrared Dust Emission from NGC 2403 and M83.” Monthly Notices of the Royal Astronomical Society, vol. 448, no. 1, Mar. 2015, pp. 168–87. EBSCOhost, https://doi.org/10.1093/mnras/stu2715.
APA
Jones, A. G., Bendo, G. J., Baes, M., Boquien, M., Boselli, A., De Looze, I., Fritz, J., Galliano, F., Hughes, T. M., Lebouteiller, V., Lu, N., Madden, S. C., Rémy-Ruyer, A., Smith, M. W. L., Spinoglio, L., & Zijlstra, A. A. (2015). The relationship between polycyclic aromatic hydrocarbon emission and far-infrared dust emission from NGC 2403 and M83. Monthly Notices of the Royal Astronomical Society, 448(1), 168–187. https://doi.org/10.1093/mnras/stu2715
Chicago
Jones, A. G., G. J. Bendo, M. Baes, M. Boquien, A. Boselli, I. De Looze, J. Fritz, et al. 2015. “The Relationship between Polycyclic Aromatic Hydrocarbon Emission and Far-Infrared Dust Emission from NGC 2403 and M83.” Monthly Notices of the Royal Astronomical Society 448 (1): 168–87. doi:10.1093/mnras/stu2715.