Cite
Optical emission line nebulae in galaxy cluster cores 1: the morphological, kinematic and spectral properties of the sample.
MLA
Hamer, S. L., et al. “Optical Emission Line Nebulae in Galaxy Cluster Cores 1: The Morphological, Kinematic and Spectral Properties of the Sample.” Monthly Notices of the Royal Astronomical Society, vol. 460, no. 2, Aug. 2016, pp. 1758–89. EBSCOhost, https://doi.org/10.1093/mnras/stw1054.
APA
Hamer, S. L., Edge, A. C., Swinbank, A. M., Wilman, R. J., Combes, F., Salomé, P., Fabian, A. C., Crawford, C. S., Russell, H. R., Hlavacek-Larrondo, J., McNamara, B. R., & Bremer, M. N. (2016). Optical emission line nebulae in galaxy cluster cores 1: the morphological, kinematic and spectral properties of the sample. Monthly Notices of the Royal Astronomical Society, 460(2), 1758–1789. https://doi.org/10.1093/mnras/stw1054
Chicago
Hamer, S. L., A. C. Edge, A. M. Swinbank, R. J. Wilman, F. Combes, P. Salomé, A. C. Fabian, et al. 2016. “Optical Emission Line Nebulae in Galaxy Cluster Cores 1: The Morphological, Kinematic and Spectral Properties of the Sample.” Monthly Notices of the Royal Astronomical Society 460 (2): 1758–89. doi:10.1093/mnras/stw1054.