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Stephens, J. R., Rusell, R. W. (1979) Emission and extinction of ground and vapor-condensed silicates from 4 to 14 microns and the 10 micron silicate feature. The Astrophysical Journal, 228. 780pp. doi:10.1086/156904

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Reference TypeJournal (article/letter/editorial)
TitleEmission and extinction of ground and vapor-condensed silicates from 4 to 14 microns and the 10 micron silicate feature
JournalThe Astrophysical Journal
AuthorsStephens, J. R.Author
Rusell, R. W.Author
Year1979 (March)Volume228
PublisherIOP Publishing
DOIdoi:10.1086/156904Search in ResearchGate
Generate Citation Formats
Mindat Ref. ID3313100Long-form Identifiermindat:1:5:3313100:1
GUID0
Full ReferenceStephens, J. R., Rusell, R. W. (1979) Emission and extinction of ground and vapor-condensed silicates from 4 to 14 microns and the 10 micron silicate feature. The Astrophysical Journal, 228. 780pp. doi:10.1086/156904
Plain TextStephens, J. R., Rusell, R. W. (1979) Emission and extinction of ground and vapor-condensed silicates from 4 to 14 microns and the 10 micron silicate feature. The Astrophysical Journal, 228. 780pp. doi:10.1086/156904
In(1979) The Astrophysical Journal Vol. 228. IOP Publishing

See Also

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Stephens, J. R. (1980) Visible and ultraviolet /800-130 nm/ extinction of vapor-condensed silicate, carbon, and silicon carbide smokes and the interstellar extinction curve. The Astrophysical Journal, 237. 450pp. doi:10.1086/157888
Puetter, R. C., Russell, R. W., Willner, S. P., Soifer, B. T. (1979) Spectrophotometry of compact H II regions from 4 to 8 microns. The Astrophysical Journal, 228. 118pp. doi:10.1086/156828
Simpson, Janet P. (1991) IRAS low-resolution spectral observations of the 10 and 18 micron silicate emission feature. The Astrophysical Journal, 368. 570pp. doi:10.1086/169721
Russell, R. W., Soifer, B. T., Forrest, W. J. (1975) Spectrophotometric observations of MU Cephei and the moon from 4 to 8 microns. The Astrophysical Journal, 198. doi:10.1086/181806
Day, K. L. (1974) A possible identification of the 10-micron ``silicate'' feature. The Astrophysical Journal, 192. doi:10.1086/181578
Jones, T. J. (1979) Polarimetry of Be stars at 1.25 and 2.2 microns. The Astrophysical Journal, 228. 787pp. doi:10.1086/156905
McCarthy, J. F., Forrest, W. J., Briotta, D. A., Jr., Houck, J. R. (1980) The galactic center - 16-30 micron observations and the 18 micron extinction. The Astrophysical Journal, 242. 965pp. doi:10.1086/158528
Hao, Lei, Spoon, H. W. W., Sloan, G. C., Marshall, J. A., Armus, L., Tielens, A. G. G. M., Sargent, B., van Bemmel, I. M., Charmandaris, V., Weedman, D. W., Houck, J. R. (2005) The Detection of Silicate Emission from Quasars at 10 and 18 Microns. The Astrophysical Journal, 625 (2). doi:10.1086/431227
Volk, Kevin, Kwok, Sun (1987) On the contribution of interstellar extinction to the 10 micron dust feature in OH/IR stars. The Astrophysical Journal, 315. 654pp. doi:10.1086/165167
Szkody, P., Raymond, J. C., Capps, R. W. (1982) The low state of AM Herculis - Observations from 0.12 to 10 microns. The Astrophysical Journal, 257. 686pp. doi:10.1086/160023
Sarazin, C. L. (1978) The effect of multiple grain components on infrared radiation transfer and the 10 micron silicate feature. The Astrophysical Journal, 220. 165pp. doi:10.1086/155892
 
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