Cmg 38
0.03
UTI
0.0
CN
0.02
Cdens
0.12
CC3
0.0
Clit
0.84
Cdup
Radius (P>50% members)
7.8 [arcmin]
- CN 0.0 Sparse
- Cdens 0.02 Very loose
- CC3 0.12 Very low quality
- Clit 0.0 Rarely studied
- Cdup 0.84 Very likely unique
Overview
Cmg 38 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a large distance, well below 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 7 years.
Note: This is very likely a unique object, which shares a small percentage of members with at least one previously reported entry. See table with shared members information.
â ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=0.84) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.
No fundamental parameters
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 78.777 | 19.936 | 0.194 | 0.275 | -1.084 | -1.297 |
| Bica et al. | 2019 | 78.824 | 19.88 | â | â | â | â |
đĄ Note: The UCC values are estimated from its identified members.
