activity
20072019
most citedA multi-transition HCN and HCO+ study of 12 nearby active galaxies: AGN versus SB environments

253 citations · 1.2k across the 19 of their papers we have counts for

collaborators

19 papers

astro-ph.HE2019★ 4 cited

GRB 190114C in the nuclear region of an interacting galaxy -- A detailed host analysis using ALMA, HST and VLT

A. de Ugarte Postigo, C. C. Thöne, S. Martın +28

GRB 190114C is the first GRB for which the detection of very-high energy emission up to the TeV range has been reported. It is still unclear whether environmental properties might…

astro-ph.GA2019★ 48 cited

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…

astro-ph.GA2019★ 56 cited

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…

astro-ph.GA2019★ 32 cited

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…

astro-ph.GA2019★ 37 cited

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…

astro-ph.HE2018★ 30 cited

The luminous host galaxy, faint supernova and rapid afterglow rebrightening of GRB 100418A

A. de Ugarte Postigo, C. C. Thoene, K. Bensch +35

Long gamma-ray bursts give us the chance to study both their extreme physics and the star-forming galaxies in which they form. GRB 100418A, at a z = 0.6239, had a bright optical an…