73 citations · 144 across the 8 of their papers we have counts for
8 papers
A Search for 3-mm Molecular Absorption Line Transitions in the Magellanic Stream
Lucille Steffes, Daniel R. Rybarczyk, Snežana Stanimirović +14
The Magellanic Stream, a tidal tail of diffuse gas falling onto the Milky Way, formed by interactions between the Small and Large Magellanic Clouds, is primarily composed of neutra…
Stellar laboratories. VII. New Kr IV - VII oscillator strengths and an improved spectral analysis of the hot, hydrogen-deficient DO-type white dwarf RE0503-289
T. Rauch, P. Quinet, D. Hoyer +4
For the spectral analysis of high-resolution and high-signal-to-noise (S/N) spectra of hot stars, state-of-the-art non-local thermodynamic equilibrium (NLTE) model atmospheres are…
High-velocity gas towards the LMC resides in the Milky Way halo
P. Richter, K. S. de Boer, K. Werner +1
To explore the origin of high-velocity gas in the direction of the Large Magellanic Cloud (LMC) we analyze absorption lines in the ultraviolet spectrum of a Galactic halo star that…
The VLT-FLAMES Tarantula Survey. IX. The interstellar medium seen through Diffuse Interstellar Bands and neutral sodium
Jacco Th. van Loon, Mandy Bailey, Benjamin L. Tatton +11
The Tarantula Nebula (30 Dor) is a spectacular star-forming region in the Large Magellanic Cloud, seen through gas in the Galactic Disc and Halo. Diffuse Interstellar Bands offer a…
On the origin of gaseous galaxy halos - Low-column density gas in the Milky Way halo
N. Ben Bekhti, B. Winkel, P. Richter +2
Recent observations show that spiral galaxies are surrounded by extended gaseous halos as predicted by the hierarchical structure formation scenario. The origin and nature of extra…
Absorption and emission line studies of gas in the Milky Way halo
N. Ben Bekhti, P. Richter, B. Winkel +4
We perform a systematic study of physical properties and distribution of neutral and ionised gas in the halo of the Milky Way (MW). Beside the large neutral intermediate- and high-…
High-resolution 21-cm observations of low-column density gas clumps in the Milky Way halo
N. Ben Bekhti, P. Richter, B. Winkel +2
We study the properties of low-column density gas clumps in the halo of the Milky Way based on high-resolution 21-cm observations. Using interferometric data from the WSRT and the…
CaII and NaI absorption signatures from the circumgalactic gas of the Milky Way
N. Ben Bekhti, M. Murphy, P. Richter +1
We combine CaII/NaI absorption and HI 21 cm emission line measurements to analyse the metal abundances, the distribution, the small-scale structure, and the physical conditions of…