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Home List of Titles The local supermassive black hole mass density: corrections for dependencies on the Hubble constant
Please use this identifier to cite or link to this item: http://hdl.handle.net/1959.3/25502
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- The local supermassive black hole mass density: corrections for dependencies on the Hubble constant
- Graham, Alister W.; Driver, Simon P.
- We have investigated past measurements of the local supermassive black hole mass density, correcting for hitherto unknown dependencies on the Hubble constant, which, in some cases, had led to an underestimation of the mass density by factors of similar to 2. Correcting for this, we note that the majority of (but not all) past studies yield a local supermassive black hole mass density that is consistent with the range 4.4 - 5.9 x 10(5) f (H-0) M circle dot Mpc(-3) when using H-0 = 70 km s(-1) Mpc(-1)). In addition, we address a number of ways in which these past estimates can be further developed. In particular, we tabulate realistic bulge-to-total flux ratios which can be used to estimate the luminosity of bulges and subsequently their central black hole masses.
- Publication type
- Journal article
- Research centre
- Swinburne University of Technology. Faculty of Information and Communication Technologies. Centre for Astrophysics and Supercomputing
- Monthly Notices of the Royal Astronomical Society: Letters, Vol. 380, no. 1 (Sep 2007), pp. L15-L19
- Publication year
- FOR Code(s)
- 0201 Astronomical and Space Sciences
- Active galactic nuclei; Black hole physics; Bulges; Cosmological parameters; Dwarf elliptic galaxies; Galaxy evolution; Luminosity function; Millennium Galaxy Catalogue; MLG; Photometry; Surface; Velocity dispersions
- Publisher URL
- Copyright © 2007 The authors. Journal copyright © 2007 Royal Astronomical Society. The accepted manuscript of the paper is reproduced here in accordance with the copyright policy of the publisher. The definitive version is available at www.interscience.wiley.com.
- Full text
- Peer reviewed