The studies of interstellar organic molecules formation in comets were discussed. The gaseous and solid composition of sources in the interstellar medium (ISM) was compared with those of the comet. The dominant chemical pathways in the grain chemistry of interstellar carbon monoxide ices were shown.
|Number of pages||4|
|Journal||European Space Agency, (Special Publication) ESA SP|
|Publication status||Published - 2002 Jul 1|
- Molecular Clouds
ASJC Scopus subject areas
- Aerospace Engineering
- Space and Planetary Science