Detection of faint BLR components in the starburst/Seyfert galaxy NGC 6221 and measure of the central BH mass

In the last decade, using single epoch virial based techniques in the optical band, it has been possible to measure the central black hole mass on large type 1 Active Galactive Nuclei (AGN) samples. However these measurements use the width of the broad line region as a proxy of the virial velocities...

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Bibliographic Details
Main Authors: Fabio eLa Franca, Francesca eOnori, Federica eRicci, Stefano eBianchi, Alessandro eMarconi, Eleonora eSani, Cristian eVignali
Format: Article
Language:English
Published: Frontiers Media S.A. 2016-04-01
Series:Frontiers in Astronomy and Space Sciences
Subjects:
Online Access:http://journal.frontiersin.org/Journal/10.3389/fspas.2016.00012/full