activity
19992017
most citedSEDIGISM: Structure, excitation, and dynamics of the inner Galactic interstellar medium

128 citations · 606 across the 13 of their papers we have counts for

collaborators

13 papers

astro-ph.GA2017★ 128 cited

SEDIGISM: Structure, excitation, and dynamics of the inner Galactic interstellar medium

F. Schuller, T. Csengeri, J. S. Urquhart +41

The origin and life-cycle of molecular clouds are still poorly constrained, despite their importance for understanding the evolution of the interstellar medium. We have carried out…

astro-ph.CO2011★ 1 cited

The sub-mm morphology of the interacting galaxy NGC 3627

M. Dumke, M. Krause, R. Beck +3

We present sub-mm continuum and heterodyne data of the interacting galaxy NGC 3627, obtained with the HHT and APEX. We find significant changes in the molecular line ratios over sm…

astro-ph.SR2010★ 11 cited

The sub-mm J=6-5 line of 13CO in Orion

T. L. Wilson, D. Muders, M. Dumke +2

We present a fully sampled map covering the Orion Hot Core and dense molecular ridge, in the sub-millimeter J=6-5 rotational transition of 13CO, at 0.45 mm with a resolution of 13…

astro-ph.CO2010★ 71 cited

PACS and SPIRE photometer maps of M33: First results of the Herschel M33 extended survey (HERM33ES)

C. Kramer, C. Buchbender, E. M. Xilouris +37

Within the framework of the HERM33ES key project, we are studying the star forming interstellar medium in the nearby, metal-poor spiral galaxy M33, exploiting the high resolution a…

astro-ph2006★ 74 cited

Probing isotopic ratios at z = 0.89: molecular line absorption in front of the quasar PKS 1830-211

Sebastien Muller, Michel Guelin, Michael Dumke +2

With the Plateau de Bure interferometer, we have measured the C, N, O and S isotopic abundance ratios in the arm of a spiral galaxy with a redshift of 0.89. The galaxy is seen face…

astro-ph2006★ 9 cited

C18O (3-2) observations of the Cometary Globule CG 12: a cold core and a C18O hot spot

L. K. Haikala, M. Juvela, J. Harju +3

The feasibility of observing the C18O (3-2) spectral line in cold clouds with the APEX telescope has been tested. As the line at 329.330 GHz lies in the wing of a strong atmospheri…