BDSB 66
(BDS2003 66)
0.13
UTI
0.0
CN
0.38
Cdens
0.25
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad)
1.9 [N/pc2]
- CN 0.0 Sparse
- Cdens 0.38 Loose
- CC3 0.25 Low quality
- Clit 0.0 Rarely studied
- Cdup 1.0 Unique
Overview
BDSB 66 is a sparse, loose object of low C3 quality. Its parallax locates it at a moderate distance, above the mid-plane. No fundamental parameter values are available for this object. It is rarely studied in the literature, with no articles listed in the last 23 years.
â ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 69.207 | 50.879 | 0.25 | -0.102 | -0.489 | 5.155 |
| Bica et al. | 2003 | 69.21 | 50.877 | â | â | â | â |
đĄ Note: The UCC values are estimated from its identified members.
MOCA

Bica et al. (2003)
Classified as infrared cluster (IRC).