165 citations · 658 across the 15 of their papers we have counts for
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The MBHBM Project -- II. Molecular Gas Kinematics in the Lenticular Galaxy NGC 3593 Reveal a Supermassive Black Hole
Dieu D. Nguyen, Martin Bureau, Sabine Thater +15
As part of the Measuring Black Holes in Below Milky Way-mass (M) galaxies (MBHBM) Project, we present a dynamical measurement of the supermassive black hole (SMBH)…
Spiral morphology in an intensely star-forming disk galaxy more than 12 billion years ago
Takafumi Tsukui, Satoru Iguchi
Spiral galaxies have distinct internal structures including a stellar bulge, disk and spiral arms. It is unknown when in cosmic history these structures formed. We analyze observat…
WISDOM Project -- IX Giant Molecular Clouds in the Lenticular Galaxy NGC4429: Effects of Shear and Tidal Forces on Clouds
Lijie Liu, Martin Bureau, Leo Blitz +5
We present high spatial resolution (12pc) Atacama Large Millimeter/sub-millimeter Array CO(J=3-2) observations of the nearby lenticular galaxy NGC4429. We identify 217 giant molecu…
WISDOM project -- VIII. Multi-scale feedback cycles in the brightest cluster galaxy NGC 0708
Eve V. North, Timothy A. Davis, Martin Bureau +8
We present high-resolution (synthesised beam size 0."088x0."083 or 25x23 pc) Atacama Large Millimetre/submillimetre Array (ALMA) CO(2-1) line and 236 GHz continuum obser…
WISDOM Project -- VII. Molecular gas measurement of the supermassive black hole mass in NGC 7052
Mark D. Smith, Martin Bureau, Timothy A. Davis +7
Supermassive black hole (SMBH) masses can be measured by resolving the dynamical influences of the SMBHs on spatially-resolved tracers of the central potentials. Modern long-baseli…
WISDOM project -- VI. Exploring the relation between supermassive black hole mass and galaxy rotation with molecular gas
Mark D. Smith, Martin Bureau, Timothy A. Davis +6
Empirical correlations between the masses of supermassive black holes (SMBHs) and properties of their host galaxies are well-established. Among these is the correlation with the fl…