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Cross-checking SMBH mass estimates in NGC 6958 -- I: Stellar dynamics from adaptive optics-assisted MUSE observations
Sabine Thater, Davor Krajnović, Peter M. Weilbacher +9
Supermassive black hole masses (MBH) can dynamically be estimated with various methods and using different kinematic tracers. Different methods have only been cross-checked for a s…
Fornax 3D project: assessing the diversity of IMF and stellar population maps within the Fornax Cluster
I. Martín-Navarro, F. Pinna, L. Coccato +14
The stellar initial mass function (IMF) is central to our interpretation of astronomical observables and to our understanding of most baryonic processes within galaxies. The univer…
The Fornax 3D project: PNe populations and stellar metallicity in edge-on galaxies
P. M. Galán-de Anta, M. Sarzi, T. W. Spriggs +17
Context. Extragalactic Planetary Nebulae (PNe) are useful distance indicators and are often used to trace the dark-matter content in external galaxies. At the same time, PNe can al…
Diversity of nuclear star cluster formation mechanisms revealed by their star formation histories
K. Fahrion, M. Lyubenova, G. van de Ven +15
Nuclear star clusters (NSCs) are the densest stellar systems in the Universe and are found in the centres of all types of galaxies. They are thought to form via mergers of star clu…
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…