activity
20192023
most citedCHIMPS2: Survey description and CO emission in the Galactic Centre

42 citations · 96 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2023★ 9 cited

Sulfur isotope ratios in the Large Magellanic Cloud

Y. Gong, C. Henkel, K. M. Menten +11

Sulfur isotope ratios have emerged as a promising tool for tracing stellar nucleosynthesis, quantifying stellar populations, and investigating the chemical evolution of galaxies. W…

astro-ph.GA2021★ 22 cited

Kinetic temperature of massive star-forming molecular clumps measured with formaldehyde IV. The ALMA view of N113 and N159W in the LMC

X. D. Tang, C. Henkel, K. M. Menten +25

We mapped the kinetic temperature structure of two massive star-forming regions, N113 and N159W, in the Large Magellanic Cloud (LMC). We have used 1\hbox{$\,.\!\!^{\prime\pri…

astro-ph.GA2020★ 42 cited

CHIMPS2: Survey description and CO emission in the Galactic Centre

D. J. Eden, T. J. T. Moore, M. J. Currie +103

The latest generation of Galactic-plane surveys is enhancing our ability to study the effects of galactic environment upon the process of star formation. We present the first data…

astro-ph.GA2020★ 9 cited

An imaging line survey of OMC-1 to OMC-3

N. Brinkmann, F. Wyrowski, J. Kauffmann +4

Aims: Our aim is to identify the dominant molecular cooling lines and characteristic emission features in the 1.3 mm window of distinct regions in the northern part of the Orion A…

astro-ph.GA2019★ 9 cited

36 GHz methanol lines from nearby galaxies: maser or quasi-thermal emission?

P. Humire, C. Henkel, Y. Gong +12

Methanol (CH3OH) is one of the most abundant interstellar molecules, offering a vast number of transitions to be studied, including many maser lines. While the strongest Galactic C…

astro-ph.GA2019★ 5 cited

Searching for further evidence for cloud-cloud collisions in L1188

Y. Gong, X. D. Tang, C. Henkel +9

In order to search for further observational evidence of cloud-cloud collisions in one of the promising candidates, L1188, we carried out observations of multiple molecular lines t…