253 citations · 1.2k across the 19 of their papers we have counts for
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Super Hot Cores in NGC 253: Witnessing the formation and early evolution of Super Star Clusters
Fernando Rico-Villas, Jesus Martin-Pintado, Eduardo Gonzalez-Alfonso +2
Using ( pc) ALMA images of vibrationally excited HCN emission (HCN) we reveal the presence of unresolved Super Hot Cores (SHCs) in the…
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…
Molecular line emission in NGC 4945, imaged with ALMA
C. Henkel, S. Muehle, G. Bendo +31
NGC 4945 is one of the nearest (~3.8 Mpc; 1" ~ 19 pc) starburst galaxies. ALMA band 3 (3--4\,mm) observations of HCN, HCO+, CS, C3H2, SiO, HCO, and CH3C2H were carried out with ~2"…
Luminous, pc-scale CO 6-5 emission in the obscured nucleus of NGC1377
S. Aalto, S. Muller, F. Costagliola +13
High resolution submm observations are important in probing the morphology, column density and dynamics of obscured active galactic nuclei (AGNs). With high resolution (0.06 x 0.05…