The masses of nuclear black holes in luminous elliptical galaxies and implications for the space density of the most massive black holes

Black hole (BH) masses predicted from the Ṁ-σ relationship conflict with predictions from the Ṁ-L relationship for high-luminosity galaxies, such as brightest cluster galaxies (BCGs). The Ṁ-L relationship predicts that some BCGs may harbor BHs with M approaching 1010 M⊙, while the Ṁ- σ relations...

Full description

Bibliographic Details
Main Authors: Lauer, T, Faber, S, Richstone, D, Gebhardt, K, Tremaine, S, Postman, M, Dressler, A, Aller, M, Filippenko, A, Green, R, Ho, L, Kormendy, J, Magorrian, J, Pinkney, J
Format: Journal article
Language:English
Published: Institute of Physics Publishing 2007