190 citations · 3.7k across the 86 of their papers we have counts for
7 papers · 2 filters
Enhanced UV radiation and dense clumps in Mrk231's molecular outflow
Claudia Cicone, Roberto Maiolino, Susanne Aalto +2
We present interferometric observations of the CN(1-0) line emission in Mrk231 and combine them with previous observations of CO and other H gas tracers to study the physical p…
ALMACAL VI: Molecular gas mass density across cosmic time via a blind search for intervening molecular absorbers
Anne Klitsch, Celine Peroux, Martin A. Zwaan +12
We are just starting to understand the physical processes driving the dramatic change in cosmic star-formation rate between and the present day. A quantity directly linke…
Chlorine-bearing molecules in molecular absorbers at intermediate redshifts
S. H. J. Wallstrom, S. Muller, E. Roueff +3
We use observations of chlorine-bearing species in molecular absorbers at intermediate redshifts to investigate chemical properties and Cl/Cl isotopic ratios in the a…
SOFIA Far-infrared [O III] and [O I] Observations of Dense CO-knots in the Supernova Remnant Cassiopeia A: Multi-phase Ejecta
Jeonghee Rho, Sofia Wallstrom, Sebastien Muller +5
Dense, fast-moving ejecta knots in supernova remnants are prime sites for molecule and dust formation. We present SOFIA far-IR spectrometer FIFI-LS observations of CO-rich knots in…
The hidden heart of the luminous infrared galaxy IC 860 I. A molecular inflow feeding opaque, extreme nuclear activity
S. Aalto, S. Muller, S. König +19
High-resolution (0."03 - 0."09) (9 - 26 pc)) ALMA (100 - 350 GHz (3 - 0.8 mm)) and VLA 45 GHz measurements have been used to image continuum and spectral line emission from the inn…
Spatially resolved carbon and oxygen isotopic ratios in NGC 253 using optically thin tracers
S. Martin, S. Muller, C. Henkel +4
To trace chemical evolution in a prototypical starburst environment, we spatially resolve the carbon and oxygen isotope ratios across the central molecular zone (full size ~$\sim 6…
Hidden or missing outflows in highly obscured galaxy nuclei?
N. Falstad, F. Hallqvist, S. Aalto +19
Understanding the nuclear growth and feedback processes in galaxies requires investigating their often obscured central regions. One way to do this is to use (sub)millimeter line e…