We use more than a decade of radial-velocity measurements for α Cen A, B, and Proxima Centauri from the High Accuracy Radial Velocity Planet Searcher, CTIO High Resolution Spectrograph, and the Ultraviolet and Visual Echelle Spectrograph to identify the M i sin and orbital periods of planets that...
Enlace original:
http://repositorio.unab.cl/xmlui/handle/ria/6357
Zhao, L.
,
Fischer, D.A.
,
Brewer, J.
,
Giguere, M.
,
Rojas-Ayala, B.
,
[Planet Detectability in the Alpha Centauri System]
,
Planet Detectability in the Alpha Centauri System
