کد مقاله کد نشریه سال انتشار مقاله انگلیسی نسخه تمام متن
5429789 1397370 2011 9 صفحه PDF دانلود رایگان
عنوان انگلیسی مقاله ISI
Stratified dust grains in the interstellar medium. III: Infrared cross-sections
موضوعات مرتبط
مهندسی و علوم پایه شیمی طیف سنجی
پیش نمایش صفحه اول مقاله
Stratified dust grains in the interstellar medium. III: Infrared cross-sections
چکیده انگلیسی

We construct a model of interstellar dust in which H-rich amorphous carbon is deposited on silicate substrates in the interstellar medium, and is annealed to form H-poor amorphous carbon. The model grains are stratified spheres composed of hollow silicate cores coated with two carbonaceous layers, the inner layer of sp2 carbon and the outer layer of sp3 carbon. Using an accurate method of computing the optical properties of such layered grains, we explore the consequences of varying the core-grain size distribution and the thicknesses of the carbonaceous layers on the resulting infrared extinction. We find a wide dispersion in the curve morphology that reflects the grain size distributions and the chemical composition of dust materials.

Research highlights► Silicate grains with carbon mantles and PAHs can fit the mean ISEC from UV to IR. ► Variations in the grain size ranges produce large variation in the IR extinction. ► Mantle chemical composition affects IR extinction. ► The degree of porosity in the grains modifies the shape of the spectral features. ► IR extinction observations may help to constrain some physical parameters in dust models.

ناشر
Database: Elsevier - ScienceDirect (ساینس دایرکت)
Journal: Journal of Quantitative Spectroscopy and Radiative Transfer - Volume 112, Issue 11, July 2011, Pages 1898-1906
نویسندگان
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