C. Brüns

The Parkes HI survey of the Magellanic System

We present the first fully and uniformly sampled, spatially complete

Deep H I observations of the compact high-velocity cloud HVC 125+41{207

\ion{H}{i}

Effelsberg HI observations of compact high-velocity clouds

survey of the entire Magellanic System with high velocity resolution (

Low-column density gas clumps in the halo of the Milky Way

\Delta v = 1.0

Dynamical evolution of high velocity clouds in the intergalactic medium

km s -1 ), performed with the Parkes Telescope. Approximately 24 percent of the southern sky was covered by this survey on a ≈ 5´ grid with an angular resolution of

Physical properties of two compact high-velocity clouds possibly associated with the leading arm of the Magellanic system

{\it HPBW} = 14\farcm1

X-Ray Searches for Emission from the WHIM in the Galactic Halo and the Intergalactic Medium

. A fully automated data-reduction scheme was developed for this survey to handle the large number of

Ca II K observations of QSOs in the line-of-sight to the Magellanic Bridge

\ion{H}{i}

Rosat x-ray sources in the field of the lmc I.total lmc gas from the background agn spectral fits

spectra (

HVCS Interacting With Their Environment

1.5\times10^6