International audienceWe report the gas-phase detection and spectroscopic characterization of ethynethiol(HCCSH), a metastable isomer of thioketene (H2C2S) using a combination of Fourier-transform microwave and submillimeter-wave spectroscopies. Severala-type transitionsof the normal species were initially detected below 40 GHz using a supersonic expansion-electrical discharge source, and subsequent measurement of higher-frequency,b-typelines using double resonance provided accurate predictions in the submillimeter region.With these, searches using a millimeter-wave absorption spectrometer equipped with aradio frequency discharge source were conducted in the range 280 – 660 GHz, ultimatelyyielding nearly 100 transitions up torR0(36) andrQ0(...
Author Institution: Department of Chemistry, University of Virginia, McCormick Rd., P.O. Box 400319,...
Context. Thioformaldehyde is an abundant molecule in various regions of the interstellar medium. How...
The ethynol (HCCOH) molecule has recently been shown to be present in simulated astrochemical ices p...
We report the gas-phase detection and spectroscopic characterisation of ethynethiol (HCCSH), a metas...
Because of their curious electronic properties, carbon-sulfide chains possess peculiar molecular st...
Context. One of the biggest unsolved mysteries of modern astrochemistry is understanding chemical fo...
Author Institution: Harvard Smithsonian Center for Astrophysics and School of Engineering and Applie...
In the course of ongoing efforts to determine accurate pure rotational transition frequencies for t...
Context. One of the biggest unsolved mysteries of modern astrochemistry is understanding chemical fo...
Context. One of the biggest unsolved mysteries of modern astrochemistry is understanding chemical fo...
A longstanding problem in astrochemistry is the inability of many current models to account for miss...
The cyclic molecule ethylene oxide (c-C_2 H_4 O) has recently been detected in the interstellar sour...
Context. Thioformaldehyde is an abundant molecule in various regions of the interstellar medium. How...
Author Institution: Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 021...
none3Methanimine (CH2NH) and ketenimine (CH2CNH) are unstable molecules which have been detected in ...
Author Institution: Department of Chemistry, University of Virginia, McCormick Rd., P.O. Box 400319,...
Context. Thioformaldehyde is an abundant molecule in various regions of the interstellar medium. How...
The ethynol (HCCOH) molecule has recently been shown to be present in simulated astrochemical ices p...
We report the gas-phase detection and spectroscopic characterisation of ethynethiol (HCCSH), a metas...
Because of their curious electronic properties, carbon-sulfide chains possess peculiar molecular st...
Context. One of the biggest unsolved mysteries of modern astrochemistry is understanding chemical fo...
Author Institution: Harvard Smithsonian Center for Astrophysics and School of Engineering and Applie...
In the course of ongoing efforts to determine accurate pure rotational transition frequencies for t...
Context. One of the biggest unsolved mysteries of modern astrochemistry is understanding chemical fo...
Context. One of the biggest unsolved mysteries of modern astrochemistry is understanding chemical fo...
A longstanding problem in astrochemistry is the inability of many current models to account for miss...
The cyclic molecule ethylene oxide (c-C_2 H_4 O) has recently been detected in the interstellar sour...
Context. Thioformaldehyde is an abundant molecule in various regions of the interstellar medium. How...
Author Institution: Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 021...
none3Methanimine (CH2NH) and ketenimine (CH2CNH) are unstable molecules which have been detected in ...
Author Institution: Department of Chemistry, University of Virginia, McCormick Rd., P.O. Box 400319,...
Context. Thioformaldehyde is an abundant molecule in various regions of the interstellar medium. How...
The ethynol (HCCOH) molecule has recently been shown to be present in simulated astrochemical ices p...