803 citations · 6.4k across the 78 of their papers we have counts for
79 papers
Tentative Detection of FeS toward Orion SrcI
Aitana Tasa-Chaveli, Holger S. P. Müller, Álvaro Sánchez-Monge +3
Iron sulfide (FeS) is a key refractory compound in astrophysical environments. It is commonly found in meteorites and evidence of FeS has only been reported in solid form in a prot…
ATOMIUM: Continuum emission and evidence of dust enhancement from binary motion
T. Danilovich, N. Samaratunge, Y. Mori +35
Low- and intermediate-mass stars on the asymptotic giant branch (AGB) account for a significant portion of the dust and chemical enrichment in their host galaxy. Here we present AL…
ATOMIUM: Molecular inventory of 17 oxygen-rich evolved stars observed with ALMA
S. H. J. Wallstrom, T. Danilovich, H. S. P. Muller +35
The dusty winds of cool evolved stars are a major contributor of the newly synthesised material enriching the Galaxy and future generations of stars. However, the details of the ph…
Millimetre and submillimetre spectroscopy of isobutene and its detection in the molecular cloud G+0.693
Mariyam Fatima, Holger S. P. Müller, Oliver Zingsheim +5
Isobutene ((CH)C=CH) is one of the four isomers of butene (CH). Given the detection of propene (CHCH=CH) toward TMC-1, and also in the warmer environmen…
Rotational spectroscopy of mono-deuterated oxirane (-CHDO) and its detection towards IRAS 162932422 B
Holger S. P. Müller, Jes K. Jørgensen, Jean-Claude Guillemin +2
We prepared a sample of mono-deuterated oxirane and studied its rotational spectrum in the laboratory between 490 GHz and 1060 GHz in order to improve its spectroscopic parameters…
(Sub)stellar companions shape the winds of evolved stars
L. Decin, M. Montargès, A. M. S. Richards +32
Binary interactions dominate the evolution of massive stars, but their role is less clear for low- and intermediate-mass stars. The evolution of a spherical wind from an asymptotic…