Numerical simulations of type III planetary migration
Planets are believed to form in primordial gas-dust discs surrounding newborn stars. An important breakthrough in our understanding of planetary formation was the discovery of extra-solar planets around sun-like stars, especially the frequent occurrence of giant planets on close orbits (hot Jupiters...
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| Format: | Doctoral Thesis |
| Language: | English |
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Stockholms universitet, Institutionen för astronomi
2008
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| Online Access: | http://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-7461 http://nbn-resolving.de/urn:isbn:978-91-7155-623-3 |