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Revealing the intermediate-mass black hole at the heart of the dwarf galaxy NGC404 with sub-parsec resolution ALMA observations

Davis, Timothy A. (författare)
Cardiff University
Nguyen, Dieu D. (författare)
National Institutes of Natural Sciences (NINS)
Seth, Anil C. (författare)
University of Utah
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Greene, Jenny E. (författare)
Princeton University
Nyland, Kristina (författare)
Naval Research Laboratory
Barth, Aaron J. (författare)
University of California at Irvine (UCI)
Bureau, Martin (författare)
Yonsei University,University Of Oxford
Cappellari, Michele (författare)
University Of Oxford
den Brok, Mark (författare)
Leibniz-Institut Für Astrophysik Potsdam,Leibniz Institute for Astrophysics Potsdam
Iguchi, Satoru (författare)
National Institutes of Natural Sciences (NINS),The Graduate University for Advanced Studies (SOKENDAI)
Lelli, Federico (författare)
Cardiff University
Liu, Lijie (författare)
University Of Oxford
Neumayer, Nadine (författare)
Max Planck Gesellschaft zur Förderung der Wissenschaften e.V. (MPG),Max Planck Society for the Advancement of Science (MPG)
North, (författare)
Cardiff University
Onishi, Kyoko, 1989 (författare)
Chalmers tekniska högskola,Chalmers University of Technology
Sarzi, Marc (författare)
Smith, Mark D. (författare)
University Of Oxford
Williams, Thomas G. (författare)
Max Planck Gesellschaft zur Förderung der Wissenschaften e.V. (MPG),Max Planck Society for the Advancement of Science (MPG)
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 (creator_code:org_t)
2020-07-14
2020
Engelska.
Ingår i: Monthly Notices of the Royal Astronomical Society. - : Oxford University Press (OUP). - 0035-8711 .- 1365-2966. ; 496:4, s. 4061-4078
  • Tidskriftsartikel (refereegranskat)
Abstract Ämnesord
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  • We estimate the mass of the intermediate-mass black hole at the heart of the dwarf elliptical galaxy NGC 404 using Atacama Large Millimetre/submillimetre Array (ALMA) observations of the molecular interstellar medium at an unprecedented linear resolution of approximate to 0.5 pc, in combination with existing stellar kinematic information. These ALMA observations reveal a central disc/torus of molecular gas clearly rotating around the black hole. This disc is surrounded by a morphologically and kinematically complex flocculent distribution of molecular clouds, that we resolve in detail. Continuum emission is detected from the central parts of NGC 404, likely arising from the Rayleigh-Jeans tail of emission from dust around the nucleus, and potentially from dusty massive star-forming clumps at discrete locations in the disc. Several dynamical measurements of the black hole mass in this system have been made in the past, but they do not agree. We show here that both the observed molecular gas and stellar kinematics independently require a approximate to 5 x 10(5) M-circle dot black hole once we include the contribution of the molecular gas to the potential. Our best estimate comes from the high-resolution molecular gas kinematics, suggesting the black hole mass of this system is 5.5(-3.8)(+4.1) x 10(5) M-circle dot (at the 99 per cent confidence level), in good agreement with our revised stellar kinematic measurement and broadly consistent with extrapolations from the black hole mass-velocity dispersion and black hole massbulge mass relations. This highlights the need to accurately determine the mass and distribution of each dynamically important component around intermediate-mass black holes when attempting to estimate their masses.

Ämnesord

NATURVETENSKAP  -- Fysik -- Subatomär fysik (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Subatomic Physics (hsv//eng)
NATURVETENSKAP  -- Kemi -- Analytisk kemi (hsv//swe)
NATURAL SCIENCES  -- Chemical Sciences -- Analytical Chemistry (hsv//eng)
NATURVETENSKAP  -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)

Nyckelord

galaxies: evolution
galaxies: dwarf
galaxies: elliptical and lenticular, cD
ISM-galaxies: kinematics and dynamics
galaxies: individual: NGC 404-galaxies

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art (ämneskategori)
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