Methyl formate in star forming regions

Details Methyl formate in star forming regions Methyl formate in star forming regions

May 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011iaus..280p.279o&link_type=abstract

The Molecular Universe, Posters from the proceedings of the 280th Symposium of the International Astronomical Union held in Tole

Astronomy and Astrophysics

Astronomy

Scientific paper

Methyl formate is an important organic complex molecule that has been detected in hot cores and hot corinos, two different regions in the interstellar medium. Chemical model based only on gas-phase reactions are unable to account for the observed abundances of methyl formate, and it is believed that gas-grain chemical models are therefore needed. We update the gas-grain model UCL/CHEM (Viti et al. 2004) to include recent experiments involving methyl formate and present in this poster a chemical model for a sample of hot cores and hot corinos. The work presented here is a part of the LASSIE European Network.

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