Astronomy and Astrophysics – Astrophysics
Scientific paper
Feb 1980
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980ap%26ss..67..495k&link_type=abstract
Astrophysics and Space Science, vol. 67, no. 2, Feb. 1980, p. 495-502.
Astronomy and Astrophysics
Astrophysics
112
Amorphous Materials, Carbon, Infrared Absorption, Interstellar Extinction, Interstellar Matter, Electron Microscopy, Far Infrared Radiation, Graphite, Microstructure, Optical Properties
Scientific paper
Extinction measurements were made for three kinds of amorphous carbon grains in the range 2100 A-340 microns. Absolute values of extinction coefficients from different sources vary by almost constant factors. Wavelength dependences of extinction curves show an inverse or less steep fall off, against an inverse-squared or steeper fall off for graphite grains. Small humps are found around 6.3, 8, 13.3 and 90 microns, although their origins are not yet clear. The infrared properties of amorphous carbon grains suggest that they could supply a significant amount of far-infrared emission noted in recent astronomical observations.
Hasegawa Hidenao
Koike Chiyoe
Manabe Atsushi
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