195 citations · 1k across the 17 of their papers we have counts for
17 papers
High-mass star formation at sub-50AU scales
H. Beuther, A. Ahmadi. J. C. Mottram, H. Linz +6
Methods: We observed the high-mass hot core region G351.77-0.54 with ALMA and more than 16km baselines. Results: At a spatial resolution of 18/40au (depending on the distance), we…
OH absorption in the first quadrant of the Milky Way as seen by THOR
M. R. Rugel, H. Beuther, S. Bihr +20
The hydroxyl radical (OH) is present in the diffuse molecular and partially atomic phases of the interstellar medium (ISM), but its abundance relative to hydrogen is not clear. We…
Magnetic fields at the onset of high-mass star formation
H. Beuther, J. Soler, W. Vlemmings +9
Context: The importance of magnetic fields at the onset of star formation related to the early fragmentation and collapse processes is largely unexplored today. Aims: We want to un…
Fragmentation and disk formation in high-mass star formation: The ALMA view of G351.77-0.54 at 0.06" resolution
H. Beuther, A. J. Walsh, K. G. Johnston +4
Aims: We resolve the small-scale structure around the high-mass hot core region G351.77-0.54 to investigate its disk and fragmentation properties. Methods: Using ALMA at 690GHz wit…
Continuum sources from the THOR survey between 1 and 2 GHz
S. Bihr, K. G. Johnston, H. Beuther +19
We carried out a large program with the Karl G. Jansky Very Large Array (VLA): "THOR: The HI, OH, Recombination line survey of the Milky Way". We observed a significant portion of…
Spectral imaging of the Central Molecular Zone in multiple 7-mm molecular lines
P. A. Jones, M. G. Burton, M. R. Cunningham +2
We have imaged 24 spectral lines in the Central Molecular Zone (CMZ) around the Galactic Centre, in the range 42 to 50 GHz. The lines include emission from the CS, CH3OH, HC3N, SiO…