Galactic halo gas traces inflowing star-formation fuel and feedback from a galaxy's disk and
is therefore crucial to our understanding of galaxy evolution. In this review, we summarize …

The Magellanic Clouds are surrounded by an extended network of gaseous structures. Chief
among these is the Magellanic Stream, an interwoven tail of filaments trailing the Clouds in …

We present a review of spatially resolved giant molecular clouds (GMCs) in nearby galaxies,
aiming at providing a template of GMC properties, which may be extrapolated to distant …

We present the first fully and uniformly sampled, spatially complete survey of the entire
Magellanic System with high velocity resolution (km s-1), performed with the Parkes …

We present an overview of the HERschel Inventory of The Agents of Galaxy Evolution
(HERITAGE) in the Magellanic Clouds project, which is a Herschel Space Observatory open …

Regions of different metallicity have been identified in the Magellanic Clouds by using the
ratio between Asymptotic Giant Branch stars of spectral type C and M. In the Large …

We present a new analysis of the diffuse gas in the Magellanic Bridge (RA≳ 3 h) based on
HST STIS E140M and FUSE spectra of two early-type stars lying within the Bridge and a …

We investigate the evolution of the interstellar medium (ISM) in self-consistent,
chemodynamical simulations of the Magellanic Clouds (MCs) during their recent (z< 0.3) …

We present the results of a new, wide-field, and broad-ranging survey for 12 CO (1-0)
emission regions in the nearest and brightest tidal structure: the Magellanic Bridge. We have …

We examine the properties of the Magellanic Bridge connecting the Large and Small
Magellanic Clouds using ab-type RR Lyrae variables from the extensive data set of the …