Search for methyl carbamate in W51e2

Details Search for methyl carbamate in W51e2 Search for methyl carbamate in W51e2

Dec 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004sf2a.conf..493d&link_type=abstract

SF2A-2004: Semaine de l'Astrophysique Francaise, meeting held in Paris, France, June 14-18, 2004. Edited by F. Combes, D. Barret

Astronomy and Astrophysics

Astrophysics

2

Scientific paper

Complex organic molecules containing up to 10 atoms have been detected in several hot molecular clouds such as Orion or SgrB2. Glycine (NH2CH2COOH), the simplest amino acid, has been extensively searched in hot cores and in molecular outflows but has not been firmly detected yet. Using the 30m IRAM antenna at Pico Veleta, we have searched for the methyl carbamate (NH2COOCH3), the isomere of glycine, in the hot molecular cloud W51e2 and in the intermediate mass protostar IRAS21391+58502. This molecule, if present in molecular clouds, should be more favorable to detect than glycine thanks to its strong dipole moment. This poster presents the results from these observations.

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