| Autor: |
Marshall, J. P., Löhne, T., Montesinos, B., Krivov, A. V., Eiroa, C., Absil, O., Bryden, G., Maldonado, J., Mora, A., Sanz-Forcada, J., Ardila, D., Augereau, J.-Ch., Bayo, A., del Burgo, C., Danchi, W., Ertel, S., Fedele, D., Fridlund, M., Lebreton, J., González-García, B. M., Liseau, R., Meeus, G., Müller, S., Pilbratt, G. L., Roberge, A., Stapelfeldt, K., Thébault, P., White, G. J., Wolf, S. |
| Zdroj: |
Astronomy and Astrophysics; May 2011, Vol. 529 Issue: 1 |
| Abstrakt: |
Context.Dusty debris discs around main sequence stars are thought to be the result of continuous collisional grinding of planetesimals in the system. The majority of these systems are unresolved and analysis of the dust properties is limited by the lack of information regarding the dust location. |
| Databáze: |
Supplemental Index |
| Externí odkaz: |
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