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A Self-Perpetuating Catalyst for the Production of Complex Organic Molecules in Protostellar Nebulae
Ist Teil von
The Astrophysical journal, 2008-02, Vol.673 (2), p.L225-L228
Ort / Verlag
Chicago, IL: IOP Publishing
Erscheinungsjahr
2008
Link zum Volltext
Quelle
EZB Electronic Journals Library
Beschreibungen/Notizen
When hydrogen, nitrogen, and CO are exposed to amorphous iron silicate surfaces at temperatures between 500 and 900 K a carbonaceous coating forms via Fischer-Tropsch-type reactions. Under normal circumstances such a coating would impede or stop further reaction. However, we find that this coating is a better catalyst than the amorphous iron silicates that initiate these reactions. Formation of a self-perpetuating catalytic coating on grain surfaces could explain the rich deposits of macromolecular carbon found in primitive meteorites and would imply that protostellar nebulae should be rich in organic material.