Amorphous carbon grains: Size effects in ultraviolet spectra
暂无分享,去创建一个
[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.