Autor:
Ramos, R.C.
Minniti, D.
Fernández-Trincado, J.G.
Alonso-Garcia, J.
Catelan, M.
Gran, F.
Hajdu, G.
Hanke, M.
Hempel, M.
Diaz, E.M.
Pérez-Villegas, A.
Rojas-Arriagada, A.
Zoccali, M.
We use deep, multi-epoch near-IR images of the VISTA Variables in the Via Lictea (VVV) Survey to measure proper motions (PMs) of stars in the Milky Way globular cluster (GC) FSR1716 = VVV-GC05. The colormagnitude diagram of this object, made by using PM-selected members, shows an extended horizon...
Enlace original:
http://repositorio.unab.cl/xmlui/handle/ria/10879
Ramos, R.C.
,
Minniti, D.
,
Fernández-Trincado, J.G.
,
Alonso-Garcia, J.
,
Catelan, M.
,
Gran, F.
,
Hajdu, G.
,
Hanke, M.
,
Hempel, M.
,
Diaz, E.M.
,
Pérez-Villegas, A.
,
Rojas-Arriagada, A.
,
Zoccali, M.
,
[The Orbit of the New Milky Way Globular Cluster FSR1716 =VVV-GC05]
,
The Orbit of the New Milky Way Globular Cluster FSR1716 =VVV-GC05
