collaborators

13 papers

astro-ph.GA2026

Massive black holes and their galaxies

Ricarda S. Beckmann, Rebecca J. Smethurst

Almost every galaxy in the local Universe is observed to have a massive black hole in the centre. The properties of these black holes are observed to tightly correlate with those o…

astro-ph.GA2026

Galaxy Zoo Bar Lengths: A Catalogue of Measurements from Hubble Space Telescope Images and the Evolution of Galactic Bar Structure at z < 1

Tenley Hutchinson-Smith, Brooke D. Simmons, Karen L. Masters +12

Understanding the role of galactic scale bars in disk galaxy evolution requires detailed measurements of bar properties across galaxies hosting bars at many redshifts. We present m…

astro-ph.GA2026

Introducing : a new universal kinematic disturbance parameter

Jonah M. Powley, Rebecca J. Smethurst, Chris J. Lintott +1

We introduce a new kinematic disturbance parameter, (pronounced `DVSG'), which takes advantage of integral field spectroscopy (IFS) to quantify differences between…

astro-ph.GA2026

The Role of Baryonic and Dark Matter in Bar Kinematics

Tobias Géron, Kai Zhu, Steph Campbell +3

Simulations predict that bars in galaxies should slow down over time. This is often attributed to the exchange of angular momentum between the bar and other regions of the galaxy,…

astro-ph.GA2026

The complex relationships between AGN, bars and bulges

Izzy L. Garland, Henry Best, Lucy F. Fortson +9

Context. Via scaling relations, it is well-known that active galactic nuclei (AGN) and bulges are linked. This link was thought to be driven by mergers, but recent studies show tha…

astro-ph.GA2026

The effects of bar strength and kinematics on galaxy evolution II: The global and local impacts of slow-strong bars

Petra Mengistu, Karen L. Masters, Tobias Geron +3

There is now clear evidence, from a variety of studies, that galactic bars contribute to and/or accelerate processes which quench galaxies. However, bars have a variety of strength…