DBSB 74
(DBSB2003 74)
0.05
UTI
0.0
CN
0.01
Cdens
0.25
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad)
0.0 [N/pc2]
- CN 0.0 Sparse
- Cdens 0.01 Very loose
- CC3 0.25 Low quality
- Clit 0.0 Rarely studied
- Cdup 1.0 Unique
Overview
DBSB 74 is a sparse, very loose object of low C3 quality. Its parallax locates it at a large distance, near 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 | 182.529 | -62.88 | 0.141 | -7.145 | 0.727 | 1.275 |
| Dutra et al. | 2003 | 182.495 | -62.832 | â | â | â | â |
đĄ Note: The UCC values are estimated from its identified members.
MOCA

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