Amorphous carbon grains: Size effects in ultraviolet spectra

[1]  L. Colangeli,et al.  Amorphous carbon and the unidentified infrared bands , 1987 .

[2]  L. Colangeli,et al.  Laboratory measurements of physical properties on submicronic particles candidate as cosmic dust , 1985 .

[3]  U. Kreibig,et al.  OPTICAL ABSORPTION OF SMALL METALLIC PARTICLES , 1985 .

[4]  F. Bassani,et al.  Size effect in the optical properties of small metallic particles: A solvable model for cubic symmetry , 1985 .

[5]  H. M. Lee,et al.  Optical properties of interstellar graphite and silicate grains , 1984 .

[6]  L. Colangeli,et al.  The absorption efficiency of submicron amorphous carbon particles between 2.5 and 40 μm , 1983 .

[7]  P. Wyder,et al.  Electronic properties of small metallic particles , 1981 .

[8]  R. Hoshino,et al.  Influence of Lattice Defects on the Width of Plasma Resonance Absorption of Silver Island Films , 1981 .

[9]  A. Manabe,et al.  Extinction coefficients of amorphous carbon grains from 2100 Å to 340 μm , 1980 .

[10]  Tetsuo Yamamoto,et al.  Grain Formation through Nucleation Process in Astrophysical Environment , 1977 .

[11]  R. Buhrman,et al.  Ultrafine metal particles , 1976 .

[12]  S. Jain,et al.  Optical properties of silver colloidal centers in KCl crystals , 1974 .

[13]  S. Yatsuya,et al.  Formation of Ultrafine Metal Particles by Gas Evaporation Technique. I. Aluminium in Helium , 1973 .

[14]  D. Huffman,et al.  Measured Extinction Efficiency of Graphite Smoke in the Region 1200–6000 Å , 1973 .

[15]  S. Yatsuya,et al.  Mean Size and Size Distribution of Metal Fine Particles Produced by Gas Evaporation Technique , 1972 .

[16]  D. Gilra,et al.  Composition of Interstellar Grains , 1970, Nature.