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A deep proper-motion survey of the nearby open cluster Blanco 1.
- Source :
-
Monthly Notices of the Royal Astronomical Society . May2011, Vol. 413 Issue 2, p1024-1035. 12p. 1 Diagram, 2 Charts, 7 Graphs. - Publication Year :
- 2011
-
Abstract
- We provide two comprehensive catalogues of positions and proper motions in the area of open cluster Blanco 1. The main catalogue, CM, contains 6271 objects down to and covers a circular ∼11 deg area. The accuracy of CM proper motions, at about 0.3-0.5 mas yr for well-measured stars, permits an excellent segregation between the cluster and field stars. The vector-point diagram of proper motions indicates an estimated total of ∼165 cluster members among the stars in our sample, while 314 stars with 2.5 mas yr have membership probabilities per cent. We also explored the astrometric potential of the Catalogue of Objects and Measured Parameters from All Sky Surveys (COMPASS) data base in order to obtain additional proper motions for fainter stars in the area of Blanco 1. This effort produced the second catalogue of proper motions, CD, containing 11 598 objects down to . A total of 4273 objects are common between the two catalogues. The accuracy of proper motions in CD ranges from 1.0 to 6 mas yr. A combination of both proper-motion catalogues was instrumental in confirming that Blanco 1 contains a large population of M dwarfs (∼150 down to M5 V - the limit of our survey). In many respects, Blanco 1 is a scaled down 'twin' of the Pleiades. The noted discrepancy between the distance from a new Hipparcos parallax of Blanco 1 and the cluster's photometric distance, at least partially, might be due to the apparent correlation between parallax and proper motion in right ascension for the ensemble of cluster members. [ABSTRACT FROM AUTHOR]
Details
- Language :
- English
- ISSN :
- 00358711
- Volume :
- 413
- Issue :
- 2
- Database :
- Academic Search Index
- Journal :
- Monthly Notices of the Royal Astronomical Society
- Publication Type :
- Academic Journal
- Accession number :
- 60154412
- Full Text :
- https://doi.org/10.1111/j.1365-2966.2011.18194.x