GLIMPSE 17
(Mercer 17)
0.03
UTI
0.0
CN
0.03
Cdens
0.38
CC3
0.0
Clit
0.4
Cdup
Radius (P>50% members)
3.6 [arcmin]
- CN 0.0 Sparse
- Cdens 0.03 Very loose
- CC3 0.38 Low quality
- Clit 0.0 Rarely studied
- Cdup 0.4 Possibly duplicate
Overview
GLIMPSE 17 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 7 years.
â ī¸ Warning: This is possibly a duplicate object, which shares a significant 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=0.4) 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 | 287.27 | 8.115 | 0.124 | -2.142 | -4.542 | 40.509 |
| Bica et al. | 2019 | 287.331 | 8.197 | â | â | â | â |
đĄ Note: The UCC values are estimated from its identified members.
