Extending the Mbh-σ diagram with dense nuclear star clusters
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
Funding
ARC | DP110103509
ARC | FT110100263
History
Available versions
PDF (Published version)Publisher DOI
ISSN
0035-8711Journal title
Monthly Notices of the Royal Astronomical SocietyVolume
422Issue
2Pagination
1586-1591Publisher
WileyCopyright statement
This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society ©: 2012 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.Language
engUsage metrics
Categories
No categories selectedKeywords
Licence
Exports
RefWorks
BibTeX
Ref. manager
Endnote
DataCite
NLM
DC