Astrominralogical studies on material circulation in the galaxy
Author:
Affiliation:
1. Department of Earth and Planetary Science, School of Science, The University of Tokyo
Publisher
Japan Association of Mineralogical Sciences
Subject
Economic Geology,Geochemistry and Petrology
Link
https://www.jstage.jst.go.jp/article/gkk/51/1/51_220225/_pdf
Reference68 articles.
1. Begemann, B., Dorschner, J., Henning, T., Mutschke, H., Guertler, J., Koempe, C. and Nass, R. (1997): Aluminum oxide and the opacity of oxygen-rich circumstellar dust in the 12-17 micron range. Astrophys. J., 476, 199-208.
2. Bouwman, J., Henning, T., Hillenbrand, L., Meyer, M., Pascucci, I., Carpenter, J., Hines, D., Kim, J., Silverstone, M. and Hollenbach, D. (2008): The formation and evolution of planetary systems: Grain growth and chemical processing of dust in T Tauri systems. Astrophys. J., 683, 479.
3. Croat, T.K., Bernatowicz, T.J. and Daulton, T.L. (2014): Presolar graphitic carbon spherules: Rocks from stars. Elements, 10, 441-446.
4. Demyk, K., d'Hendecourt, L., Leroux, H., Jones, A.P. and Borg, J. (2004): IR spectroscopic study of olivine, enstatite and diopside irradiated with low energy H+ and He+ ions. Astron. Astrophys., 420, 233-243.
5. Dorschner, J. (1971a): Dust production in circumstellar space. Astronomische Nachrichten, 293, 65-70.
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