Autor:
Kurtev, R.
Gromadzki, M.
Beamín, J.C.
Folkes, S.L.
Pena Ramirez, K.
Ivanov, V.D.
Borissova, J.
Villanueva, V.
Minniti, D.
Mendez, R.
Lucas, P.W.
Smith, L.C.
Pinfield, D.J.
Kuhn, M.A.
Jones, H.R.A.
Antonova, A.
Yip, A.K.P.
Knowledge of the stellar content near the Sun is important for a broad range of topics ranging from the search for planets to the study of Milky Way (MW) structure. The most powerful method for identifying potentially nearby stars is proper motion (PM) surveys. All old optical surveys avoid, or a...
Enlace original:
http://repositorio.unab.cl/xmlui/handle/ria/4243
Kurtev, R.
,
Gromadzki, M.
,
Beamín, J.C.
,
Folkes, S.L.
,
Pena Ramirez, K.
,
Ivanov, V.D.
,
Borissova, J.
,
Villanueva, V.
,
Minniti, D.
,
Mendez, R.
,
Lucas, P.W.
,
Smith, L.C.
,
Pinfield, D.J.
,
Kuhn, M.A.
,
Jones, H.R.A.
,
Antonova, A.
,
Yip, A.K.P.
,
[VVV high proper motion stars – I. The catalogue of bright KS ≤ 13.5 stars]
,
VVV high proper motion stars – I. The catalogue of bright KS ≤ 13.5 stars
