Volume 429, Number 1, January I 2005
|Page(s)||205 - 208|
|Section||Interstellar and circumstellar matter|
|Published online||13 December 2004|
Crystalline MgSiO and amorphous Mg-bearing silicate grain formation by coalescence and growth
Department of Nanophysics in Frontier Projects, Ritsumeikan University, Kusatsu-shi, Shiga 525-8577, Japan e-mail: email@example.com
2 Laboratory for Extraterrestrial Physics, Code 691, NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA
3 Department of Electronics and Information Science, Kyoto Institute of Technology, Matsugasaki, Sakyo-ku, Kyoto 606-8585, Japan
Accepted: 23 August 2004
A novel method for producing MgO and SiO2 smokes was developed. Mg-bearing silicate grain formation using the coalescence and growth of MgO and SiO2 grains was carried out in our laboratory. It becomes evident that single and poly crystalline Mg2SiO4 (forsterite) and amorphous Mg-bearing silicate grains can be produced by the coalescence and growth of MgO and SiO2 grains. This result suggests that the observed crystalline Mg2SiO4 grains and amorphous Mg-bearing silicate particles in Red Super Giant (RSG), Asymptotic Giant Branch (AGB), post-AGB and planetary nebula (PNe) could be produced by the coalescence and growth of MgO and SiO2 grains.
Key words: astrochemistry / methods: laboratory / stars: AGB and post-AGB / circumstellar matter / dust, extinction
© ESO, 2005
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