806 citations · 15.8k across the 221 of their papers we have counts for
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Large scale IRAM 30m CO-observations in the giant molecular cloud complex W43
P. Carlhoff, Q. Nguyen Luong, P. Schilke +11
We aim to give a full description of the distribution and location of dense molecular clouds in the giant molecular cloud complex W43. It has previously been identified as one of t…
Complex organic molecules in the interstellar medium: IRAM 30 m line survey of Sagittarius B2(N) and (M)
Arnaud Belloche, Holger S. P. Müller, Karl M. Menten +2
The discovery of amino acids in meteorites and the detection of glycine in samples returned from a comet to Earth suggest that the interstellar chemistry is capable of producing su…
Ionization toward the high-mass star-forming region NGC 6334 I
J. L. Morales Ortiz, C. Ceccarelli, D. C. Lis +3
Context. Ionization plays a central role in the gas-phase chemistry of molecular clouds. Since ions are coupled with magnetic fields, which can in turn counteract gravitational col…
Interstellar detection of c-C3D2
S. Spezzano, S. Brünken, P. Schilke +7
We report the first interstellar detection of c-C3D2. The doubly deuterated cyclopropenylidene, a carbene, has been detected toward the starless cores TMC- 1C and L1544 using the I…
Spectral imaging of the Central Molecular Zone in multiple 7-mm molecular lines
P. A. Jones, M. G. Burton, M. R. Cunningham +2
We have imaged 24 spectral lines in the Central Molecular Zone (CMZ) around the Galactic Centre, in the range 42 to 50 GHz. The lines include emission from the CS, CH3OH, HC3N, SiO…
Dimethyl ether in its ground state, v=0, and lowest two torsionally excited states, v11=1 and v15=1, in the high-mass star-forming region G327.3-0.6
Suzanne E. Bisschop, Peter Schilke, Friedrich Wyrowski +11
The goal of this paper is to determine the respective importance of solid state vs. gas phase reactions for the formation of dimethyl ether. This is done by a detailed analysis of…