Authors:
Grishko, VI
Tereszchuk, K
Duley, WW
Bernath, P
Citation: Vi. Grishko et al., The far-infrared spectrum of hydrogenated amorphous carbon and the 21, 27,and 33 micron features in carbon-rich proto-planetary nebulae, ASTROPHYS J, 558(2), 2001, pp. L129-L132
Citation: Ww. Duley et Vi. Grishko, Evolution of carbon dust in aromatic infrared emission sources: Formation of nanodiamonds, ASTROPHYS J, 554(2), 2001, pp. L209-L212
Citation: Ww. Duley, The 3.3 micron and extended red emissions in interstellar clouds: Further evidence for carbon nanoparticles, ASTROPHYS J, 553(2), 2001, pp. 575-580
Citation: Vi. Grishko et Ww. Duley, Detection of new infrared spectral features in hydrogenated amorphous carbon, ASTROPHYS J, 543(1), 2000, pp. L85-L88
Citation: Ss. Seahra et Ww. Duley, Normal coordinate analysis and vibrational spectra of aromatic carbon nanostructures, ASTROPHYS J, 542(2), 2000, pp. 898-913
Authors:
Maldoni, MM
Robinson, G
Smith, RG
Duley, WW
Scott, A
Citation: Mm. Maldoni et al., Measurements of the 44-mu m band of H2O ice deposited on amorphous carbon and amorphous silicate substrates, M NOT R AST, 309(2), 1999, pp. 325-331
Citation: Ww. Duley et Ss. Seahra, 2175 angstrom and 3.4 micron absorption bands and carbon depletion in the diffuse interstellar medium, ASTROPHYS J, 522(2), 1999, pp. L129-L132
Citation: Ww. Duley, Optical emission at 5800 angstrom in the Red Rectangle and the 5797-angstrom diffuse interstellar band, M NOT R AST, 301(4), 1998, pp. 955-959
Citation: Ww. Duley et S. Seahra, Graphite, polycyclic aromatic hydrocarbons, and the 2175 angstrom extinction feature, ASTROPHYS J, 507(2), 1998, pp. 874-888