The slope of the black hole mass versus velocity dispersion correlation

Observations of nearby galaxies reveal a strong correlation between the mass of the central dark object MBH and the velocity dispersion σ of the host galaxy, of the form log(MBH/M⊙) = α + βlog(σ/σ0); however, published estimates of the slope β span a wide range (3.75-5.3). Merritt and Ferrarese have...

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Bibliographic Details
Main Authors: Tremaine, S, Gebhardt, K, Bender, R, Bower, G, Dressler, A, Faber, S, Filippenko, A, Green, R, Grillmair, C, Ho, L, Kormendy, J, Lauer, T, Magorrian, J, Pinkney, J, Richstone, D
Format: Journal article
Language:English
Published: 2002