803 citations · 6.4k across the 78 of their papers we have counts for
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An observational study of dust nucleation in Mira ( Ceti): II. Titanium oxides are negligible for nucleation at high temperatures
T. Kamiński, H. S. P. Müller, M. R. Schmidt +7
The formation of silicate dust in oxygen-rich envelopes of evolved stars is thought to be initiated by formation of seed particles that can withstand the high temperatures close to…
Submillimeter spectroscopy of HCO and a revisit of the rotational spectra of HCO and HCO
Holger S. P. Müller, Frank Lewen
The rotational spectrum of the formaldehyde isotopologue HCO was investigated between 0.56 and 1.50 THz using a sample of natural isotopic composition. In addition, tran…
OH+ and H2O+ absorption toward PKS1830-211
S. Muller, H. S. P. M"uller, J. H. Black +13
We report the detection of OH+ and H2O+ in the z=0.89 absorber toward the lensed quasar PKS1830-211. The abundance ratio of OH+ and H2O+ is used to quantify the molecular hydrogen…
Laboratory spectroscopic study and astronomical detection of vibrationally excited n-propyl cyanide
Holger S. P. Müller, Adam Walters, Nadine Wehres +8
We performed a spectral line survey called Exploring Molecular Complexity with ALMA (EMoCA) toward Sagittarius~B2(N) between 84.1 and 114.4 GHz with the Atacama Large Millimeter/su…
Analysis of the Herschel/HEXOS Spectral Survey Towards Orion South: A massive protostellar envelope with strong external irradiation
K. Tahani, R. Plume, E. A. Bergin +14
We present results from a comprehensive submillimeter spectral survey toward the source Orion South, based on data obtained with the HIFI instrument aboard the \textit{Herschel Spa…
The ALMA Protostellar Interferometric Line Survey (PILS): First results from an unbiased submillimeter wavelength line survey of the Class 0 protostellar binary IRAS 16293-2422 with ALMA
J. K. Jørgensen, M. H. D. van der Wiel, A. Coutens +14
The inner regions of the envelopes surrounding young protostars are characterised by a complex chemistry, with prebiotic molecules present on the scales where protoplanetary disks…