Fadely, R., Willman, B., Geha, M., Walsh, S., Munoz, R., Jerjen, H., . . . Da Costa, G. (2011). Segue 3: An Old, Extremely Low Luminosity Star Cluster in the Milky Way's Halo. Institute of Physics Publishing, Inc.
Chicago Style (17th ed.) CitationFadely, R., B. Willman, M. Geha, S. Walsh, R. Munoz, H. Jerjen, L. Vargas, and G. Da Costa. Segue 3: An Old, Extremely Low Luminosity Star Cluster in the Milky Way's Halo. Institute of Physics Publishing, Inc, 2011.
MLA (9th ed.) CitationFadely, R., et al. Segue 3: An Old, Extremely Low Luminosity Star Cluster in the Milky Way's Halo. Institute of Physics Publishing, Inc, 2011.
Warning: These citations may not always be 100% accurate.