[astro-ph.GA] This study focuses on propanethiol (or propyl mercaptan, C3H7SH), a sulfur analogue of propanol and a key target for investigating interstellar sulfur chemistry. We report the laboratory rotational spectroscopic […]
molecular cloud G+0.693-0.027
New Insights Into The Origins Of The Chemistry Of Life
Researchers at the Max Planck Institute for Extraterrestrial Physics (MPE), in collaboration with astrophysicists from the Centro de Astrobiología (CAB), CSIC-INTA, have identified the largest sulfur-bearing molecule ever found in […]
Formation Of The Glycine Isomer Glycolamide (NH2C(O)CH2OH) On The Surfaces Of Interstellar Ice Grains: Insights From Atomistic Simulations
Syn-glycolamide, a glycine isomer, has recently been detected in the G+0.693-0.027 molecular cloud. Investigations on its formation in the interstellar medium could offer insights into synthetic routes leading to glycine […]
Gas-phase Formation Routes Of Dimethyl Sulfide In The Interstellar Medium
Context: Dimethyl sulfide (DMS; CH3SCH3) is an organosulfur compound that has been suggested as a potential biosignature in exoplanetary atmospheres. In addition to its tentative detections toward the sub-Neptune planet […]
On the Abiotic Origin of Dimethyl Sulfide: Discovery of DMS in the Interstellar Medium
Following the discovery of dimethyl sulfide (CH3SCH3, DMS) signatures in comet 67P/Churyumov-Gerasimenko, we report the first detection of this organosulfur species in the interstellar medium, during the exploration of an […]
What Drives The Formation Of Unsaturated Molecules In The Interstellar Medium?
We present a computational investigation into the fragmentation pathways of ethanolamine (C2H7NO, EtA), propanol (C3H8O, PrO), butanenitrile (C4H7N, BuN), and glycolamide (C2H5NO2, GlA)—saturated organic molecules detected in the interstellar medium […]
Experimental and Computational Study of Ethanolamine Ices at Astrochemical Conditions
Ethanolamine (NH2CH2CH2OH) has recently been identified in the molecular cloud G+0.693-0.027, situated in the SgrB2 complex in the Galactic center. However, its presence in other regions, and in particular in […]
Discovery Of Thionylimide, HNSO, In Space: The First N-, S- and O-bearing Interstellar Molecule
We present the first detection in space of thionylimide (HNSO) toward the Galactic Center molecular cloud G+0.693-0.027, thanks to the superb sensitivity of an ultradeep molecular line survey carried out […]
Accurate Ab Initio Spectroscopic Studies Of Promising Interstellar Ethanolamine Iminic Precursors
Context. The detection of NH2CH2CH2OH (ethanolamine) in molecular cloud G+0.693-0.027 adds an additional player to the prebiotic molecules discovered so far in the interstellar medium (ISM). As this molecule might […]
