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Estimating black hole masses in quasars using broad optical and UV emission lines

โœ Scribed by Paola Marziani; Jack W. Sulentic


Book ID
113821216
Publisher
Elsevier Science
Year
2012
Tongue
English
Weight
815 KB
Volume
56
Category
Article
ISSN
1387-6473

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## Abstract The correlation between black hole masses and stellar velocity dispersions provides an efficient method to determine the masses of black holes in active galaxies. We obtained optical spectra of a Compactโ€Steepโ€Spectrum (CSS) galaxy 4C +29.70, using the Canadaโ€Franceโ€Hawaii Telescope (CF