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Sökning: id:"swepub:oai:research.chalmers.se:ef43c148-e73d-4460-8e58-a8d26b694fc7" > Cross-checking SMBH...

Cross-checking SMBH mass estimates in NGC 6958-I. Stellar dynamics from adaptive optics-assisted MUSE observations

Thater, Sabine (författare)
Universität Wien,University of Vienna,Leibniz-Institut Für Astrophysik Potsdam,Leibniz Institute for Astrophysics Potsdam
Krajnovic, Davor (författare)
Leibniz-Institut Für Astrophysik Potsdam,Leibniz Institute for Astrophysics Potsdam
Weilbacher, Peter M. (författare)
Leibniz-Institut Für Astrophysik Potsdam,Leibniz Institute for Astrophysics Potsdam
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Nguyen, Dieu D. (författare)
Vietnam National University
Bureau, Martin (författare)
Yonsei University,University Of Oxford
Cappellari, Michele (författare)
University Of Oxford
Davis, Timothy A. (författare)
Cardiff University
Iguchi, Satoru (författare)
National Institutes of Natural Sciences (NINS)
McDermid, Richard (författare)
Macquarie University
Onishi, Kyoko, 1989 (författare)
Chalmers tekniska högskola,Chalmers University of Technology
Sarzi, Marc (författare)
van de Ven, Glenn (författare)
Universität Wien,University of Vienna
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 (creator_code:org_t)
2021-11-10
2022
Engelska.
Ingår i: Monthly Notices of the Royal Astronomical Society. - : Oxford University Press (OUP). - 0035-8711 .- 1365-2966. ; 509:4, s. 5416-5436
  • Tidskriftsartikel (refereegranskat)
Abstract Ämnesord
Stäng  
  • Supermassive black hole masses (M (BH)) can dynamically be estimated with various methods and using different kinematic tracers. Different methods have only been cross-checked for a small number of galaxies and often show discrepancies. To understand these discrepancies, detailed cross-comparisons of additional galaxies are needed. We present the first part of our cross-comparison between stellar- and gas-based M-BH estimates in the nearby fast-rotating early-type galaxy NGC 6958. The measurements presented here are based on ground-layer adaptive optics-assisted Multi-Unit Spectroscopic Explorer (MUSE) science verification data at around 0."6 spatial resolution. The spatial resolution is a key ingredient for the measurement and we provide a Gaussian parametrization of the adaptive optics-assisted point spread function for various wavelengths. From the MUSE data, we extracted the stellar kinematics and constructed dynamical models. Using an axisymmetric Schwarzschild technique, we measured an M-BH of (3.6(-2.4)(+2.7)) x10(8) M-circle dot at 3 sigma significance taking kinematical and dynamical systematics (e.g. radially varying mass-to-light ratio) into account. We also added a dark halo, but our data do not allow us to constrain the dark matter fraction. Adding dark matter with an abundance matching prior results in a 25 per cent more massive black hole. Jeans anisotropic models return M-BH of (4.6(-2.7)(+2.5)) x10(8) and (8.6(-0.8)(+0.8)) x10(8) M-circle dot at 3 sigma confidence for spherical and cylindrical alignments of the velocity ellipsoid, respectively. In a follow-up study, we will compare the stellar-based M (BH) with those from cold and warm gas tracers, which will provide additional constraints for the M-BH for NGC 6958, and insights into assumptions that lead to potential systematic uncertainty.

Ämnesord

NATURVETENSKAP  -- Fysik -- Subatomär fysik (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Subatomic Physics (hsv//eng)
NATURVETENSKAP  -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)
NATURVETENSKAP  -- Geovetenskap och miljövetenskap -- Geofysik (hsv//swe)
NATURAL SCIENCES  -- Earth and Related Environmental Sciences -- Geophysics (hsv//eng)

Nyckelord

galaxies: kinematics and dynamics
galaxies: individual: NGC 6958
galaxies: nuclei

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