Astronomy and Astrophysics – Astrophysics
Scientific paper
Jul 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989apj...342l..91b&link_type=abstract
Astrophysical Journal, Part 2 - Letters (ISSN 0004-637X), vol. 342, July 15, 1989, p. L91-L93. Research supported by NSERC.
Astronomy and Astrophysics
Astrophysics
11
Hydrocarbons, Interstellar Chemistry, Interstellar Matter, Silicon, Aromatic Compounds, Catalysis, Ground State, Isomers, Laboratories
Scientific paper
Results are reported from laboratory simulations of the formation of Si-containing interstellar molecules by the interaction of Si atoms with PAH molecules (represented by naphthalene). Data obtained in the selected-ion flow tube of the Ion Chemistry Laboratory at York University are presented in a table and briefly characterized. The implications of the results for the interstellar roles of larger PAH molecules and for reactions catalyzed by graphitic grain surfaces are indicated.
Bohme Diethard K.
Wincel H.
Wlodek Stanislaw
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