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 budget and accounting of metals in and around star-forming galaxies at z∼ 0.
We combine empirically derived star formation histories with updated supernova and …

ABSTRACT The Parkes Galactic All-Sky Survey (GASS) is a survey of Galactic atomic
hydrogen (H i) emission in the Southern sky covering declinations δ⩽ 1 using the Parkes …

We report the results of a FUSE study of high-velocity O VI absorption along complete sight
lines through the Galactic halo in directions toward 100 extragalactic objects and two halo …

ABSTRACT The Magellanic Stream is a 100 &j0;× 10 &j0; filament of gas that lies within the
Galactic halo and contains∼ 2× 10 8 M⊙ of neutral hydrogen. In this paper we present data …

ABSTRACT Green Bank Telescope 21 cm observations have revealed a faint, yet extensive
HI cloud population surrounding the Andromeda galaxy (M31). The newfound objects are …

We model the kinematics of the high-and intermediate-velocity clouds (HVCs and IVCs)
observed in absorption towards a sample of 55 Galactic halo stars with accurate distance …

We have used the Westerbork array to carry out an unbiased wide-field survey of H i
emission features, achieving an rms sensitivity of about 18 mJy/Beam at a velocity resolution …

Context. The Milky Way is surrounded by large amounts of diffuse gaseous matter that
connects the stellar body of our Galaxy with its large-scale Local Group (LG) environment …