885 citations · 11.7k across the 140 of their papers we have counts for
140 papers
The Black Hole-Galaxy Connection: Interplay between Feedback, Obscuration, and Host Galaxy Substructure
Stéphanie Juneau, Andy D. Goulding, Julie Banfield +20
There is growing evidence for physical influence between supermassive black holes and their host galaxies. We present a case study of nearby galaxy NGC 7582, for which we find evid…
The spatially-resolved gas and dust connection in neutral inflows and outflows in nearby AGN
David S. N. Rupke, Adam D. Thomas, Michael A. Dopita
Dusty, neutral outflows and inflows are a common feature of nearby star-forming galaxies. We characterize these flows in eight galaxies -- mostly AGN -- selected for their widespre…
On the origin of nitrogen at low metallicity
Arpita Roy, Michael A. Dopita, Mark R. Krumholz +3
Understanding the evolution of the N/O ratio in the interstellar medium (ISM) of galaxies is essential if we are to complete our picture of the chemical evolution of galaxies at hi…
What Drives the Redshift Evolution of Strong Emission Line Ratios?
Fuyan Bian, Lisa J. Kewley, Brent Groves +1
We study the physical mechanisms that cause the offset between low-redshift and high-redshift galaxies on the [OIII]/H versus [NII]/H ``Baldwin, Phillips & Terlevich'' (BPT)…
Theoretical ISM pressure and electron density diagnostics for local and high-redshift galaxies
Lisa J. Kewley, David C. Nicholls, Ralph S. Sutherland +4
We derive new self-consistent theoretical UV, optical, and IR diagnostics for the ISM pressure and electron density in the ionized nebulae of star-forming galaxies. Our UV diagnost…
Helium and Nitrogen Enrichment in Massive Main Sequence Stars: Mechanisms and Implications for the Origin of WNL Stars
Arpita Roy, Ralph S Sutherland, Mark R Krumholz +2
The evolutionary paths taken by massive stars with remain substantially uncertain. They begin their lives as main sequence (MS) O-stars. Dependin…