The formation of giant planets in wide orbits by photoevaporation-synchronised migration
The discovery of giant planets in wide orbits represents a major challenge for planet formation theory. In the standard core accretion paradigm planets are expected to form at radial distances ≾ 20 au in order to form massive cores (with masses ≿ 10 M®) able to trigger the gaseous runaway growth bef...
Guardado en:
| Autores principales: | Guilera, Octavio Miguel, Miller Bertolami, Marcelo Miguel, Ronco, María Paula |
|---|---|
| Formato: | Articulo Preprint |
| Lenguaje: | Español |
| Publicado: |
2017
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| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/82333 |
| Aporte de: |
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