Lw. Beegle et al., EXPERIMENTAL INDICATION OF A NAPHTHALENE-BASE MOLECULAR AGGREGATE FORTHE CARRIER OF THE 2175-ANGSTROM INTERSTELLAR EXTINCTION FEATURE, The Astrophysical journal, 487(2), 1997, pp. 976-982
Experiments where the simple polycyclic aromatic hydrocarbon (PAH) nap
hthalene (C10H8) is subjected to the energetic environment of a plasma
have resulted in the synthesis of a molecular aggregate that has ultr
aviolet spectral characteristics that suggest it provides insight into
the nature of the carrier of the 2175 Angstrom interstellar extinctio
n feature and may be a laboratory analog. Ultraviolet, visible, infrar
ed, and mass spectroscopy, along with gas chromatography, indicate tha
t it is a molecular aggregate in which an aromatic double ring (''naph
thaalene'') structural base serves as the electron ''box'' chromophore
that gives rise to the envelope of the 2175 Angstrom feature. This ch
romophore can also provide the peak of the feature or function as a ma
ntle in concert with another peak provider such as graphite. The molec
ular base/chromophore manifests itself both as a structural component
of an alkyl-aromatic polymer and as a substructure of hydrogenated PAH
species. Its spectral and molecular characteristics are consistent wi
th what is generally expected for a complex molecular aggregate that h
as a role as an interstellar constituent.