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Please use this identifier to cite or link to this item: http://hdl.handle.net/1959.3/219190
- Title
- Extending the Mbh-sigma diagram with dense nuclear star clusters
- Author(s)
- Graham, Alister W.
- Abstract
- Four new nuclear star cluster masses, Mnc, plus seven upper limits, are provided for galaxies wth previously determined black hole masses, Mbh. Together with a sample of 64 galaxies wth direct Mbh measurements, 13 of which additionally now have Mnc measurements rather than only upper limits, plus an additional 29 dwarf galaxies with available Mnc measurements and velocity dispersions
- Publication type
- Journal article
- Research centre
- Swinburne University of Technology. Faculty of Information and Communication Technologies. Centre for Astrophysics and Supercomputing
- Source
- Monthly Notices of the Royal Astronomical Society, Vol. 422, no. 2 (May 2012), pp. 1586-1591
- Publication year
- 2012
- FOR Code(s)
- 0201 Astronomical and Space Sciences
- Keyword(s)
- Dwarf galaxies; Dynamics; Fundamental parameters; Galactic nuclei; Galaxy structure; Kinematics; Star clusters
- Publisher
- Wiley-Blackwell Publishing
- ISSN
- 0035-8711
- Publisher URL
- http://dx.doi.org/10.1111/j.1365-2966.2012.20734.x
- Copyright
- Copyright © 2012 The Author. Monthly Notices of the Royal Astronomical Society copyright © 2012 RAS.
- Research Projects
-
Massive black holes in dense star clusters, Australian Research Council grant number DP110103509
The hearts of galaxies, Australian Research Council grant number FT110100263
- Peer reviewed
