Our MUSE observations of LABn06, a Ly-alpha nebula at z~3.2, indicate that it is powered by an active galactic nucleus

We are finding that the velocity widths of absorption lines around galaxies in the DIISC sample are correlated with column densities along those lines of sight

Using velocity structure functions we constrain the turbulence in extended QSO host nebulae revealed by [OII] and [OIII] emission lines

Using a class of neural networks known as a Recurrent Inference Machine, we have successfully deconvolved the source’s intrinsic spectrum from the instrumental response function for the first time.

An investigation of gamma-ray production by hadronic interaction between cosmic-ray protons and the CGM

Statistics of CIV absorbers imply large envelopes of metal-enriched gas surrounding massive galaxies

Tracking the simulated Local Group CGM and modeling Milky Way contamination in mock observations of M31

Observational evidence of a extended co-rotating disc + a galactic outflow on scales of several tens of kpc

An analysis of stacked eROSITA galaxy observations

Observations indicate that the CGM along the minor axis is on average more enriched than the gas located along the major axis of galaxies - consistent with outflow and accretion models

A brief overview of the results of Moser et al. 2022.

Atmospheric wave dynamics in the simulations of Choudhury & Reynolds (2022, arXiv:2202.05289)

A video summarising the results of Acharya & Khaire (2022, MNRAS, 509, 5559)

A video summarizing the results of Sameer et al. (2022, MNRAS, 510, 5796)

In a new paper (Buie II et al. 2022, ApJ, in press), we extend our previous CGM models to include angular momentum and MHD

This video describes the main results from Lochhaas et al. (2021, ApJ, 922, 121)

This short video reviews an upcoming publication by UW Postdoc Kirill Tchernyshyov

This video summarizes a recent paper (Voit 2021, ApJL, 908, L16) that tries to build an intuitive understanding of precipitation phenomena using schematic diagrams.