Terrestrial planets and water delivery around low-mass stars
Context. Theoretical and observational studies suggest that protoplanetary disks with a wide range of masses could be found around low-mass stars. Aims. We analyze planetary formation processes in systems without gas giants around M3- and M0-type stars of 0.29 M⊙ and 0.5 M⊙, respectively. In parti...
Guardado en:
| Autores principales: | Dugaro, Agustín, Elía, Gonzalo Carlos de, Brunini, Adrián, Guilera, Octavio Miguel |
|---|---|
| Formato: | Articulo |
| Lenguaje: | Inglés |
| Publicado: |
2016
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| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/85757 |
| Aporte de: |
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