Interstellar polycyclic aromatic hydrocarbons and carbon in interplanetary dust particles and meteorites

Science (New York, N.Y.)
|July 3, 1987
PubMed
Summary

Interplanetary dust particles and meteorites contain carbonaceous material similar to polycyclic aromatic hydrocarbons (PAHs). These findings suggest PAHs in space may form in stellar dust shells and undergo minimal interstellar modification.

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