AFGL5182
0.20
UTI
0.44
CN
0.19
Cdens
0.38
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad)
0.9 [N/pc2]
- CN 0.44 Poorly populated
- Cdens 0.19 Very loose
- CC3 0.38 Low quality
- Clit 0.0 Rarely studied
- Cdup 1.0 Unique
Overview
AFGL5182 is a poorly populated, very 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.
Note: This object shares a small percentage of members with at least one entry reported in the same catalogue. See table with shared members information.
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 | 92.222 | 21.86 | 0.426 | -0.176 | -1.636 | 30.872 |
| Bica et al. | 2003 | 92.267 | 21.843 | 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).