| Full text | |
| Author(s): |
Dias, W. S.
[1, 2]
;
Monteiro, H.
[2]
;
Caetano, T. C.
[1, 2]
;
Lepine, J. R. D.
[1]
;
Assafin, M.
[3]
;
Oliveira, A. F.
[2]
Total Authors: 6
|
| Affiliation: | [1] Univ Sao Paulo, Inst Astron Geofis & Ciencias Atmosfer, Sao Paulo - Brazil
[2] Univ Fed Itajuba, Inst Ciencias Exatas, UNIFEI, BR-37500903 Itajuba, MG - Brazil
[3] Univ Fed Rio de Janeiro, Observ Valongo, BR-20080090 Rio de Janeiro, RJ - Brazil
Total Affiliations: 3
|
| Document type: | Journal article |
| Source: | Astronomy & Astrophysics; v. 564, APR 2014. |
| Web of Science Citations: | 61 |
| Abstract | |
We present a catalog of mean proper motions and membership probabilities of individual stars for optically visible open clusters, which have been determined using data from the UCAC4 catalog in a homogeneous way. The mean proper motion of the cluster and the membership probabilities of the stars in the region of each cluster were determined by applying the statistical method in a modified fashion. In this study, we applied a global optimization procedure to fit the observed distribution of proper motions with two overlapping normal bivariate frequency functions, which also take the individual proper motion errors into account. For 724 clusters, this is the first determination of proper motion, and for the whole sample, we present results with a much larger number of identified astrometric member stars. Furthermore, it was possible to estimate the mean radial velocity of 364 clusters (102 unpublished so far) with the stellar membership using published radial velocity catalogs. These results provide an increase of 30% and 19% in the sample of open clusters with a determined mean absolute proper motion and mean radial velocity, respectively. (AU) | |
| FAPESP's process: | 13/01115-6 - A study of the galactic structure by means of open clusters |
| Grantee: | Jacques Raymond Daniel Lépine |
| Support Opportunities: | Research Grants - Visiting Researcher Grant - Brazil |