Graphite di-layers and the interstellar polycyclic aromatic hydrocarbon hypothesis

Details Graphite di-layers and the interstellar polycyclic aromatic hydrocarbon hypothesis Graphite di-layers and the interstellar polycyclic aromatic hydrocarbon hypothesis

Jan 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989apj...336l..37t&link_type=abstract

Astrophysical Journal, Part 2 - Letters (ISSN 0004-637X), vol. 336, Jan. 1, 1989, p. L37-L39.

Astronomy and Astrophysics

Astrophysics

7

Aromatic Compounds, Cyclic Hydrocarbons, Graphite, Interstellar Matter, Astronomical Spectroscopy, Energy Bands, Lattice Parameters

Scientific paper

Relative to crystalline graphite, a graphite two-layer is uniaxially compressed, and has stronger interplanar binding and substantially altered one-electron properties. These results may be relevant to astrophysical invocation of polycyclic aromatic hydrocarbons (graphitic molecules) and graphite as sources of certain emission and absorption features of the interstellar medium.

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