Hydrogenation of solid hydrogen cyanide HCN and methanimine CH2NH at low temperature
- P. Theulé, F. Borget, T. Chiavassa
- Chemistry
- 1 October 2011
Context. Hydrogenation reactions dominate grain surface chemistry in dense molecular clouds and lead to the formation of complex saturated molecules in the interstellar medium. Aims. We investigate…
A rigorous detection of interstellar CH3NCO: An important missing species in astrochemical networks.
- J. Cernicharo, Z. Kisiel, J. Guillemin
- Physics, ChemistryAstronomy & Astrophysics
- 1 March 2016
The recent analysis of the composition of the frozen surface of comet 67P/Churyumov-Gerasimenko has revealed a significant number of complex organic molecules. Methyl isocyanate (CH3NCO) is one of…
Report and implications of the first observation of C4N2 in laboratory simulations of Titan’s atmosphere
- P. Coll, J. Guillemin, M. Gazeau, F. Raulin
- Physics, Environmental Science
- 15 December 1999
Organic chemistry in Titan's atmosphere: new data from laboratory simulations at low temperature.
- P. Coll, D. Coscia, M. Gazeau, E. de Vanssay, J. Guillemin, F. Raulin
- ChemistryAdvances in Space Research
- 1995
Searching for trans ethyl methyl ether in Orion KL.
- B. Tercero, J. Cernicharo, J. Guillemin
- PhysicsAstronomy & Astrophysics
- 1 September 2015
We report on the tentative detection of trans ethyl methyl ether (tEME), t-CH3CH2OCH3, through the identification of a large number of rotational lines from each one of the spin states of the…
ALMA Detection of Interstellar Methoxymethanol (CH3OCH2OH)
- B. McGuire, C. Shingledecker, A. Remijan
- Physics
- 8 December 2017
We report the detection of interstellar methoxymethanol (CH3OCH2OH) in Atacama Large Millimeter/submillimeter Array (ALMA) Bands 6 and 7 toward the MM1 core in the high-mass star-forming region NGC…
Temperature dependence of HC3N, C6H2, and C4N2 mid-UV absorption coefficients. Application to the interpretation of Titan's atmospheric spectra
- Y. Bénilan, D. Andrieux, C. Cossart-Magos
- Physics
- 1 February 1996
Three organic compounds (HC3N, C6H2, and C4N2) relevant of Titan's atmosphere have been studied within the framework of the SIPAT (Spectroscopie UV d'Intérêt Prébiologique dans l'Atmosphère de Titan)…
Ultraviolet and infrared spectrum of C6H2 revisited and vapor pressure curve in Titan's atmosphere
- F. Shindo, Y. Bénilan, J. Guillemin, P. Chaquin, A. Jolly, F. Raulin
- Physics
- 2003
IR Spectrum of C8H2: Integrated Band Intensities and Some Observational Implications
- F. Shindo, Y. Bénilan, P. Chaquin, J. Guillemin, A. Jolly, F. Raulin
- Physics, Chemistry
- 1 December 2001
Polyynes are of astrophysical interest since they appear to be involved in organic chemistry in very different mediums. In Titan's atmosphere, the lightest polyyne, C4H2, was detected by Voyager.…
Precursors of the RNA World in Space: Detection of (Z)-1,2-ethenediol in the Interstellar Medium, a Key Intermediate in Sugar Formation
- V. Rivilla, L. Colzi, C. Puzzarini
- PhysicsAstrophysical Journal Letters
- 28 March 2022
We present the first detection of (Z)-1,2-ethenediol, (CHOH)2, the enol form of glycolaldehyde, in the interstellar medium toward the G+0.693−0.027 molecular cloud located in the Galactic Center. We…
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