Particle Shapes and the 2175 Angstroms Feature

Details Particle Shapes and the 2175 Angstroms Feature Particle Shapes and the 2175 Angstroms Feature

May 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998aas...192.4012w&link_type=abstract

American Astronomical Society, 192nd AAS Meeting, #40.12; Bulletin of the American Astronomical Society, Vol. 30, p.870

Astronomy and Astrophysics

Astronomy

Scientific paper

The galactic interstellar extinction curve exhibits a pronounced feature at 2175 Angstroms . The most striking characteristic of this feature is the relatively fixed nature of its central wavelength while the width of the feature may vary. Small graphite particles are often proposed as the carrier of this UV bump. However, graphite grains of a single size and shape cannot reproduce the observed width and peak characteristics simultaneously. Here we investigate to what extent these characteristics may be reproduced by invoking a shape distribution of prolate and oblate graphite particles. The graphite constants calculated by Draine and Lee (ApJ,285,99) do not yield the narrowest 2175 Angstroms features that have been observed. We have recalculated the dielectric function of astronomical graphite such that a spherical grain of radius 50 Angstroms produces a feature with a peak at x_0=4.6 inverse microns and gamma =0.8 . Using grains in the Rayleigh approximation, we wave calculated extinction curves for combinations of prolate, spherical, and oblate grain shapes, and successfully reproduced the stationary nature of the peak. In addition, such shape variations do give variations in the width of the feature whose relative magnitudes match the observations. However, the absolute values of the calculated widths fall short by approximately 10 percent compared with observed widths.

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