X-ray nuclear activity in S4G barred galaxies: No link between bar strength and co-occurrent supermassive black hole fueling

MLA

Cisternas, Mauricio, et al. X-Ray Nuclear Activity in S4G Barred Galaxies: No Link between Bar Strength and Co-Occurrent Supermassive Black Hole Fueling. 2013. EBSCOhost, https://doi.org/10.1088/0004-637X/776/1/50.

APA

Cisternas, M., Gadotti, D., Knapen, J. H., Kim, T., Díaz-García, S., Laurikainen, E., Salo, H., González-Martín, O., Ho, L. C., Elmegreen, B. G., Zaritsky, D., Sheth, K., Athanassoula, E., Bosma, A., Comerón, S., Erroz-Ferrer, S., De Paz, A. G., Hinz, J. L., Holwerda, B. W., … Seibert, M. (2013). X-ray nuclear activity in S4G barred galaxies: No link between bar strength and co-occurrent supermassive black hole fueling. https://doi.org/10.1088/0004-637X/776/1/50

Chicago

Cisternas, Mauricio, Dimitri Gadotti, Johan H. Knapen, Taehyun Kim, Simón Díaz-García, Eija Laurikainen, Heikki Salo, et al. 2013. “X-Ray Nuclear Activity in S4G Barred Galaxies: No Link between Bar Strength and Co-Occurrent Supermassive Black Hole Fueling.” doi:10.1088/0004-637X/776/1/50.