Fonte: Co-evolution of central black holes and galaxies. Proceedings. Nome do evento: IAU Symposium. Unidade: IAG
Assuntos: GALÁXIAS SEY FERT, POPULAÇÕES ESTELARES, GALÁXIAS ATIVAS
ABNT
RIFFEL, Rogério et al. Near-infrared spectral energy distributions of Seyfert Galaxies: stellar population, active nucleus, and hot dust. 2010, Anais.. Cambridge: Cambridge University Press, 2010. . Acesso em: 02 set. 2024.APA
Riffel, R., Pastoriza, M. G., Carciofi, A. C., Rodríguez-Ardila, A., & Bonatto, C. (2010). Near-infrared spectral energy distributions of Seyfert Galaxies: stellar population, active nucleus, and hot dust. In Co-evolution of central black holes and galaxies. Proceedings. Cambridge: Cambridge University Press.NLM
Riffel R, Pastoriza MG, Carciofi AC, Rodríguez-Ardila A, Bonatto C. Near-infrared spectral energy distributions of Seyfert Galaxies: stellar population, active nucleus, and hot dust. Co-evolution of central black holes and galaxies. Proceedings. 2010 ;[citado 2024 set. 02 ]Vancouver
Riffel R, Pastoriza MG, Carciofi AC, Rodríguez-Ardila A, Bonatto C. Near-infrared spectral energy distributions of Seyfert Galaxies: stellar population, active nucleus, and hot dust. Co-evolution of central black holes and galaxies. Proceedings. 2010 ;[citado 2024 set. 02 ]