1. One possible origin of ethanol in interstellar medium: Photochemistry of mixed CO2–C2H6 films at 11K. A FTIR study
- Author
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Pascale Ehrenfreund, L. Schriver-Mazzuoli, André Schriver, and L. d’Hendecourt
- Subjects
Astrochemistry ,Chemistry ,Infrared ,Interstellar ice ,Interstellar cloud ,General Physics and Astronomy ,Photochemistry ,Spectral line ,Interstellar medium ,Protostar ,Astrophysics::Earth and Planetary Astrophysics ,Physics::Chemical Physics ,Physical and Theoretical Chemistry ,Fourier transform infrared spectroscopy ,Astrophysics::Galaxy Astrophysics - Abstract
It has been predicted by theoretical models that ethane and ethanol are present in icy mantles covering dust particles in dense interstellar clouds. Laboratory spectra of ethanol embedded in astrophysically relevant ice matrices were compared to the Infrared Space Observatory and ground-based astronomical spectra of high mass protostars. From this comparison strict upper-limits of ethanol (compared to solid water) on interstellar grains could be derived that are below 1.2%. In dense star forming regions ethanol is observed in gas phase with an abundance which is many orders of magnitude in excess of predictions based on pure gas-phase chemistry. Ethane has not been observed in the interstellar gas or on grains. In contrast, ethane has been detected in several comets with a percentage of
- Published
- 2007
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