Host bulge properties: The key to SMBH mass estimates?

Details Host bulge properties: The key to SMBH mass estimates? Host bulge properties: The key to SMBH mass estimates?

Nov 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004iaus..222...73b&link_type=abstract

The Interplay among Black Holes, Stars and ISM in Galactic Nuclei, Proceedings of IAU Symposium, No. 222. Edited by T. Storchi-B

Physics

Scientific paper

Results gathered to anchor the MBH-σ* relation raise concerns in the methods of measuring of σ* used for the original slope determinations. We present these preliminary results to demonstrate the problem and briefly outline where the discrepancies arise. IFS is a valuable tool in addressing this area and will allow us to remove systematics before tightening the MBH-σ* relation and end the `aperture arguments'.

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