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- W2022672720 abstract "There is a tight M−σ relation in nearby inactive galaxies. Nearby radio-quiet AGNs also followed this relation. In order to investigate whether radio-loud AGNs and NLS1s follow this relation or not, we estimated their central black hole masses from Hβ and the bulge velocity dispersions from [O III] linewidth. We found that radio-loud AGNs and NLS1s seemed to deviate from this relation.To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html" @default.
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- W2022672720 date "2004-03-01" @default.
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- W2022672720 title "M-σ relation in radio-loud AGNs and NLS1s" @default.
- W2022672720 doi "https://doi.org/10.1017/s1743921304001528" @default.
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