Towards a physical model of dust tori in Active Galactic Nuclei.

MLA

Schartmann, Marc, et al. “Towards a Physical Model of Dust Tori in Active Galactic Nuclei.” AIP Conference Proceedings, vol. 761, no. 1, Apr. 2005, pp. 277–80. EBSCOhost, https://doi.org/10.1063/1.1913940.

APA

Schartmann, M., Meisenheimer, K., Camenzind, M., Wolf, S., & Henning, T. (2005). Towards a physical model of dust tori in Active Galactic Nuclei. AIP Conference Proceedings, 761(1), 277–280. https://doi.org/10.1063/1.1913940

Chicago

Schartmann, Marc, Klaus Meisenheimer, Max Camenzind, Sebastian Wolf, and Thomas Henning. 2005. “Towards a Physical Model of Dust Tori in Active Galactic Nuclei.” AIP Conference Proceedings 761 (1): 277–80. doi:10.1063/1.1913940.