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WISDOM Project – III: Molecular gas measurement of the supermassive black hole mass in the barred lenticular galaxy NGC4429

Davis, Timothy, Bureau, Martin, Onishi, Kyoko, Van de Voort, Freeke, Cappellari, Michele, Iguchi, Satoru, Liu, Lijie, North, Eve, Sarzi, Marc and Smith, Mark D. 2018. WISDOM Project – III: Molecular gas measurement of the supermassive black hole mass in the barred lenticular galaxy NGC4429. Monthly Notices of the Royal Astronomical Society 437 (3) , pp. 3818-3834. 10.1093/mnras/stx2600

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Abstract

As part of the mm-Wave Interferometric Survey of Dark Object Masses (WISDOM) project we present an estimate of the mass of the supermassive black hole (SMBH) in the nearby fast-rotating early-type galaxy NGC4429, that is barred and has a boxy/peanut-shaped bulge. This estimate is based on Atacama Large Millimeter/submillimeter Array (ALMA) cycle-2 observations of the 12CO(3–2) emission line with a linear resolution of �13 pc (0:0018 � 0:0014). NGC4429 has a relaxed, flocculent nuclear disc of molecular gas that is truncated at small radii, likely due to the combined effects of gas stability and tidal shear. The warm/dense 12CO(3-2) emitting gas is confined to the inner parts of this disc, likely again because the gas becomes more stable at larger radii, preventing star formation. The gas disc has a low velocity dispersion of 2.2+0:68

Item Type: Article
Date Type: Publication
Status: Published
Schools: Physics and Astronomy
Subjects: Q Science > QB Astronomy
Publisher: Oxford University Press
ISSN: 0035-8711
Funders: STFC
Date of First Compliant Deposit: 5 October 2017
Date of Acceptance: 4 October 2017
Last Modified: 25 Feb 2019 23:38
URI: http://orca.cf.ac.uk/id/eprint/105181

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