GLIMPSE 39
(Mercer 39)
0.01
UTI
0.0
CN
0.1
Cdens
0.12
CC3
0.0
Clit
0.24
Cdup
Radius (P>50% members)
7.6 [arcmin]
- CN 0.0 Sparse
- Cdens 0.1 Very loose
- CC3 0.12 Very low quality
- Clit 0.0 Rarely studied
- Cdup 0.24 Likely duplicate
Overview
GLIMPSE 39 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a moderate 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 7 years.
â ī¸ Warning: This is likely a duplicate object, which shares a large 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=0.24) 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 | 206.889 | -62.785 | 0.379 | -5.308 | -1.066 | â |
| Bica et al. | 2019 | 206.831 | -62.792 | â | â | â | â |
đĄ Note: The UCC values are estimated from its identified members.
