Dust growth in protoplanetary disks
Dust growth by aggregation is an important process as the first step of planet formation in protoplanetary disks. Dust growth also influences the temperature structure in protoplanetary disks. However, we still have a large uncertainty in the dust growth process. This uncertainty mainly comes from u...
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| Veröffentlicht in: | Exoplanets and disks their formation and diversity : proceedings of the international conference, Kailua-Kona, Hawaii, 9-12 March 2009 Kailua-Kona, Hawaii, 9-12 March 2009, 2009-03, Vol.1158, p.97-102 |
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| Hauptverfasser: | , , |
| Format: | Artikel |
| Sprache: | eng |
| Online-Zugang: | Volltext |
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| Zusammenfassung: | Dust growth by aggregation is an important process as the first step of planet formation in protoplanetary disks. Dust growth also influences the temperature structure in protoplanetary disks. However, we still have a large uncertainty in the dust growth process. This uncertainty mainly comes from unknown factors in dust structure. In recent years, many theoretical studies on aggregate collisions and growth have been done. In this paper, we will introduce remarkable results in these theoretical studies, mainly focusing on results by our group. |
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| ISSN: | 0094-243X |