In: Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 43, no. 3
F. Pozo Nuñez - M. Ramolla - C. Westhues - M. Haas - R. Chini - K. Steenbrugge - R. Lemke - M. Murphy
Detaily:
Rok, strany: 2014, 357 - 361
Kľúčové slová:
galaxies: active —galaxies: Seyfert —quasars: emission lines —galaxies: distances and redshifts —galaxies: individual: ESO399-IG20 —galaxies: individual: 3C120 —galaxies: individual: WPVS48
URL originálneho zdroja: http://www.astro.sk/caosp/Eedition/Abstracts/2014/Vol_43/No_3/pp357-361_abstract.html
O článku:
Photometric reverberation mapping (PRM) is a novel method used to study the geometry of the broad emission-line region (BLR), black hole masses and host-subtracted luminosities of active galactic nuclei (AGN). We obtained high-quality sampling data with small (15 to 80 cm) robotic telescopes at the observatory of the Ruhr-University Bochum, located in the Atacama desert in Chile.
Ako citovať:
ISO 690:
Pozo Nuñez, F., Ramolla, M., Westhues, C., Haas, M., Chini, R., Steenbrugge, K., Lemke, R., Murphy, M. 2014. The BLR structure and dust torus size of AGN - Implications from photometric and dust reverberation mapping campaigns.. In Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 43, no.3, pp. 357-361. 1335-1842.
APA:
Pozo Nuñez, F., Ramolla, M., Westhues, C., Haas, M., Chini, R., Steenbrugge, K., Lemke, R., Murphy, M. (2014). The BLR structure and dust torus size of AGN - Implications from photometric and dust reverberation mapping campaigns.. Contributions of the Astronomical Observatory Skalnaté Pleso, 43(3), 357-361. 1335-1842.