A Photo-Ionization Method for Black Hole Mass Estimation in Quasars

Abstract: Determining the masses of the central compact object believed to power all active galactic nuclei is relevant to our understanding of their evolution and of their inner workings. Keys to present-day mass estimates are: (1) the assumption of line broadening due to virial motion of the emitting gas, (2) an estimate of the distance of broad-line emitting gas from the central compact object, and (3) a measure of the AGN luminosity. We discuss the merits and the limitations of an alternative method based on estimates of physical conditions in the broad line emitting region derived from an appropriate multi-component analysis of emission line profiles. This ‘photo-ionization method’, applied to UV intermediate-ionization lines appears to be promising for at least a sizable population of high-z quasars.

Object Details

• Location: Deutsche Nationalbibliothek Frankfurt am Main
• Extent: Online-Ressource
• Language: Englisch

References and Relationships

• Bibliographic citation: A Photo-Ionization Method for Black Hole Mass Estimation in Quasars ; volume:20 ; number:3 ; year:2011 ; pages:406-413 ; extent:8 ; Open astronomy ; 20, Heft 3 (2011), 406-413 (gesamt 8)

Contributors, Places and Time

• Creator: Marziani, Paola ; Negrete, C. Alenka ; Dultzin, Deborah ; Sulentic, Jack W.

Further information

• DOI: 10.1515/astro-2017-0311
• URN: urn:nbn:de:101:1-2405271655204.991788338627
• Rights: Open Access; Der Zugriff auf das Objekt ist unbeschränkt möglich.
• Last update: 14.08.2025, 10:44 AM CEST