A possible activity cycle in Proxima Centauri
Context. Several late-type stars present activity cycles resembling the Solar one. This fact has been observed mostly in stars ranging from F to K, i.e., in stars with a radiative core and an outer convective layer. Aims. This work aims at studying whether an activity cycle can be detected in the dM...
Guardado en:
| Autores principales: | Cincunegui, C., Díaz, R.F., Mauas, P.J.D. |
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| Formato: | JOUR |
| Materias: | |
| Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_00046361_v461_n3_p1107_Cincunegui |
| Aporte de: |
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