Please use this identifier to cite or link to this item: http://hdl.handle.net/2381/38299
Title: The M-sigma Relation for Nucleated Galaxies
Authors: McLaughlin, Dean E.
King, Andrew R.
Nayakshin, Sergei
First Published: 20-Sep-2006
Publisher: American Astronomical Society, IOP Publishing
Citation: Astrophysical Journal Letters, 650, pp. L37-L40
Abstract: Momentum feedback from super-Eddington accretion offers a simple explanation for the observed M-sigma and M-M_{spheroid} relations between supermassive black holes (SMBH) and the spheroids of their host galaxies. Recently Ferrarese et al. and Wehner & Harris observed analogous relations between the masses of central star clusters and their hosts. We show that stellar winds and supernovae from such nuclear clusters (NC) give similar feedback explanations for this case also, and we discuss the connection to the Faber-Jackson relation for the spheroids themselves.
DOI Link: 10.1086/508627
ISSN: 2041-8205
eISSN: 2041-8213
Links: http://iopscience.iop.org/article/10.1086/508627/meta
http://hdl.handle.net/2381/38299
Version: Publisher Version
Status: Peer-reviewed
Type: Journal Article
Rights: Archived with reference to SHERPA/RoMEO and publisher website.
Description: Added reference to J. Rossa et al. (2006, AJ, 132, 1074) matching published version. ApJ Letters, in press (Vol. 650, 2006 October)
Appears in Collections:Published Articles, Dept. of Physics and Astronomy

Files in This Item:
File Description SizeFormat 
20872.web.pdfPublished (publisher PDF)63.85 kBAdobe PDFView/Open


Items in LRA are protected by copyright, with all rights reserved, unless otherwise indicated.