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12 papers · 2 filters
Paramagnetic alignment of small grains: a novel method for measuring interstellar magnetic fields
Thiem Hoang, A. Lazarian, P. G. Martin
We present a novel method to measure the strength of interstellar magnetic fields based on ultraviolet (UV) polarization of starlight, which is in part produced by weakly aligned,…
Infrared-Faint Radio Sources are at high redshifts
Andreas Herzog, Enno Middelberg, Ray P. Norris +3
Context: Infrared-Faint Radio Sources (IFRS) are characterised by relatively high radio flux densities and associated faint or even absent infrared and optical counterparts. The re…
Evidence for an Interaction in the Nearest Starbursting Dwarf Irregular Galaxy IC 10
David L. Nidever, Trisha Ashley, Colin T. Slater +10
Using deep 21-cm HI data from the Green Bank Telescope we have detected an ~18.3 kpc-long gaseous extension associated with the starbursting dwarf galaxy IC 10. The newly-found fea…
High-resolution absorption spectroscopy of the circumgalactic medium of the Milky Way
P. Richter, A. J. Fox, N. Ben Bekhti +3
In this article we discuss the importance of high-resolution absorption spectroscopy for our understanding of the distribution and physical nature of the gaseous circumgalactic med…
Studying Galactic interstellar turbulence through fluctuations in synchrotron emission: First LOFAR Galactic foreground detection
M. Iacobelli, M. Haverkorn, E. Orrú +85
The characteristic outer scale of turbulence and the ratio of the random to ordered components of the magnetic field are key parameters to characterise magnetic turbulence in the i…
CEN34 -- High-Mass YSO in M17 or Background Post-AGB Star?
Zhiwei Chen, Dieter Nuernberger, Rolf Chini +3
We investigate the proposed high-mass young stellar object (YSO) candidate CEN34, thought to be associated with the star forming region M17. Its optical to near-infrared (550-2500…