Add to ORKGNew infrared spectra are presented for H2S and four other sulfur-containing compounds, all thiols, at 10140 K to aid in the study of interstellar and solar system ices. Infrared spectral changes on warming H2S and each thiol are described with an emphasis on the SH stretching vibration at 25502525 cm(exp -1) (=3.923.96 m) as it is in a relatively unobscured part of the infrared spectra of interstellar and planetary ices. Infrared positions and band strengths for each thiols SH and CH stretching vibrations are reported, along with the SH band strength of H2S. Two band strengths of near-infrared features of CH3SH are included. Results for these compounds are compared, and some areas of agreement and disagreement with the literature are descri...
Context. Sulfur-containing molecules constitute only 8% of the molecules observed in the interstella...
This is a proposal for laboratory measurements of the infrared (λ=1- 20 μm) optical constants of hyd...
Context. Infrared spectroscopy of star and planet forming regions is at the dawn of a new age with t...
Among the most commonly existing thiol molecules, methanethiol and ethanethiol were discovered in th...
The techniques of low temperature spectroscopy are applied to identify the constituents of the ices ...
Context. Sulfur is an abundant element in the cosmos and it is thus an important contributor to astr...
Three solid phases of CH3SH (methanethiol or methyl mercaptan) have been prepared and their mid-infr...
The infrared spectrum of sulfur dioxide is of interest both for the earth (volcanic eruptions in par...
Aims. This work aims to study the unexplained sulfur depletion observed toward dense clouds and prot...
Interstellar CH4 may consume a fair amount of the carbon budget in dense molecular clouds, but proba...
This work was supported in part by The Air Force Cambridge Research Laboratories under a contract wi...
We study several molecules that could help in the solution of the missing sulfur problem in dense cl...
Author Institution: Department of Physics, The Ohio State UniversityAn extension of the transition a...
Context. Whereas observational astronomy now routinely extends to the far-infrared region of the spe...
International audienceWe present the results of the irradiation of interstellar ice analogs (H 2 O:N...
Context. Sulfur-containing molecules constitute only 8% of the molecules observed in the interstella...
This is a proposal for laboratory measurements of the infrared (λ=1- 20 μm) optical constants of hyd...
Context. Infrared spectroscopy of star and planet forming regions is at the dawn of a new age with t...
Among the most commonly existing thiol molecules, methanethiol and ethanethiol were discovered in th...
The techniques of low temperature spectroscopy are applied to identify the constituents of the ices ...
Context. Sulfur is an abundant element in the cosmos and it is thus an important contributor to astr...
Three solid phases of CH3SH (methanethiol or methyl mercaptan) have been prepared and their mid-infr...
The infrared spectrum of sulfur dioxide is of interest both for the earth (volcanic eruptions in par...
Aims. This work aims to study the unexplained sulfur depletion observed toward dense clouds and prot...
Interstellar CH4 may consume a fair amount of the carbon budget in dense molecular clouds, but proba...
This work was supported in part by The Air Force Cambridge Research Laboratories under a contract wi...
We study several molecules that could help in the solution of the missing sulfur problem in dense cl...
Author Institution: Department of Physics, The Ohio State UniversityAn extension of the transition a...
Context. Whereas observational astronomy now routinely extends to the far-infrared region of the spe...
International audienceWe present the results of the irradiation of interstellar ice analogs (H 2 O:N...
Context. Sulfur-containing molecules constitute only 8% of the molecules observed in the interstella...
This is a proposal for laboratory measurements of the infrared (λ=1- 20 μm) optical constants of hyd...
Context. Infrared spectroscopy of star and planet forming regions is at the dawn of a new age with t...