Searching for intermediate mass black holes: understanding the data first. Issue Volume 10:Issue S312(2014) (7th March 2016)

• Record Type: Journal Article
• Authors: Bianchini, Paolo; Norris, Mark; van de Ven, Glenn; Schinnerer, Eva
• Editors: Meiron, Y.; Li, S.; Liu, F.-K.; Spurzem, R.
• Is Part Of: Proceedings of the International Astronomical Union. Volume 10:Issue S312(2014)
• Page Start: 223
• Page End: 226
• Publication Date: 2016-03-07
• Subjects: black hole physics, -- globular clusters: general, -- stars: kinematics, -- instrumentation: spectrographs; Astronomy -- Congresses; Astronomy -- Periodicals; 520
• DOI: 10.1017/S174392131500784X
• Languages: English
• ISSNs: 1743-9213

Abstract

Abstract: The detection of intermediate mass black holes (IMBHs) in globular clusters has been hotly debated, with different observational methods delivering different outcomes for the same object. In order to understand these discrepancies, we construct detailed mock integral field spectroscopy (IFU) observations of globular clusters, starting from realistic Monte Carlo cluster simulations. The output is a data cube of spectra in a given field-of-view that can be analyzed in the same manner as real observations and compared to other (resolved) kinematic measurement methods. We show that the main discrepancies arise because the luminosity-weighted IFU observations can be strongly biased by the presence of a few bright stars that introduce a scatter in velocity dispersion measurements of several km s −1 . We show that this intrinsic scatter can prevent a sound assessment of the central kinematics, and therefore should be fully taken into account to correctly interpret the signature of an IMBH.