117 citations · 404 across the 7 of their papers we have counts for
9 papers
Spatially resolved star formation and fuelling in galaxy interactions
Jorge Moreno, Paul Torrey, Sara L. Ellison +8
We investigate the spatial structure and evolution of star formation and the interstellar medium (ISM) in interacting galaxies. We use an extensive suite of parsec-scale galaxy mer…
Interacting galaxies in the IllustrisTNG simulations -- I: Triggered star formation in a cosmological context
David R. Patton, Kieran D. Wilson, Colin J. Metrow +7
We use the IllustrisTNG cosmological hydrodynamical simulations to investigate how the specific star formation rates (sSFRs) of massive galaxies depend on…
Interacting galaxies in the IllustrisTNG simulations -- II: Star formation in the post-merger stage
Maan H. Hani, Hayman Gosain, Sara L. Ellison +2
Galaxy mergers are a major evolutionary transformation whose effects are borne out by a plethora of observations and numerical simulations. However, most previous simulations have…
Variations in the slope of the resolved star-forming main sequence: a tool for constraining the mass of star-forming regions
Maan H. Hani, Christopher C. Hayward, Matthew E. Orr +5
The correlation between galaxies' integrated stellar masses and star formation rates (the `star formation main sequence'; SFMS) is a well-established scaling relation. Recently, su…
Deep learning predictions of galaxy merger stage and the importance of observational realism
Connor Bottrell, Maan H. Hani, Hossen Teimoorinia +7
Machine learning is becoming a popular tool to quantify galaxy morphologies and identify mergers. However, this technique relies on using an appropriate set of training data to be…
The diversity of the circumgalactic medium around z = 0 Milky Way-mass galaxies from the Auriga simulations
Maan H. Hani, Sara L. Ellison, Martin Sparre +4
Galaxies are surrounded by massive gas reservoirs (i.e. the circumgalactic medium; CGM) which play a key role in their evolution. The properties of the CGM, which are dependent on…