Paper
25 February 2000 Physical modeling of interstellar dust
Boris S. Luk'yanchuk, Armando Luches, Armando Blanco, V. Orofino
Author Affiliations +
Proceedings Volume 4070, ALT '99 International Conference on Advanced Laser Technologies; (2000) https://doi.org/10.1117/12.378151
Event: ALT'99 International Conference: Advanced Laser Technologies, 1999, Potenza-Lecce, Italy
Abstract
Carbon nanoparticles, prepared by means of ns-laser ablation of carbon can be used for physical modeling of the interstellar dust. Different model for formation of interstellar dust were suggested for the last years, one assumes that carbon grains are generated by condensation in the expanding carbon-rich stellar plasma/vapor of cool red giants. Similar conditions for condensation can be reproduced in laser experiments. Calculations and experiments show that carbon particles produced by laser have the same size and extinction that can be seen in diffusive clouds of hydrogen-pure stars. The situation with hydrogen-rich stars is more complex: the most probable mechanism suggests that firstly the nanodiamonds are formed within these clouds which later transform to carbon onions due to annealing and graphitization.
© (2000) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Boris S. Luk'yanchuk, Armando Luches, Armando Blanco, and V. Orofino "Physical modeling of interstellar dust", Proc. SPIE 4070, ALT '99 International Conference on Advanced Laser Technologies, (25 February 2000); https://doi.org/10.1117/12.378151
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Cited by 3 scholarly publications.
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KEYWORDS
Carbon

Particles

Clouds

Diamond

Atmospheric particles

Modeling

Stars

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