The chemical complexity of hot corinos

Details The chemical complexity of hot corinos The chemical complexity of hot corinos

Jan 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005esasp.577..449b&link_type=abstract

In: Proceedings of the dusty and molecular universe: a prelude to Herschel and ALMA, 27-29 October 2004, Paris, France. Ed. by A

Computer Science

Corinos

Scientific paper

The study of hot corinos, the low-mass analogs of massive hot cores, is essential to understand the advant of life in our Solar System and to define the conditions that should prevail in the protostellar stage in order for life to develop in a planetary system. Indeed, it is during this phase that complex organic (prebiotic) molecules are formed. Here, we present initial results on the only two known hot corinos: IRAS 16293-2422 and NGC 1333-IRAS4A.

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