Schartmann, M., Meisenheimer, K., Camenzind, M., Wolf, S., & Henning, T. (2005). Towards a physical model of dust tori in active galactic nuclei. The spectral energy distributions of gas-rich galaxies. https://doi.org/10.1063/1.1913940
Chicago Style (17th ed.) CitationSchartmann, Marc, Klaus Meisenheimer, Max Camenzind, Sebastian Wolf, and Thomas Henning. "Towards a Physical Model of Dust Tori in Active Galactic Nuclei." The Spectral Energy Distributions of Gas-rich Galaxies 2005. https://doi.org/10.1063/1.1913940.
MLA (9th ed.) CitationSchartmann, Marc, et al. "Towards a Physical Model of Dust Tori in Active Galactic Nuclei." The Spectral Energy Distributions of Gas-rich Galaxies, 2005, https://doi.org/10.1063/1.1913940.
Warning: These citations may not always be 100% accurate.