GLIMPSE 13
(Mercer 13)
Summary
GLIMPSE 13 is a sparse, very loose object of low C3 quality. It is located at a large distance from the Sun, near the mid-plane. It is rarely studied in the literature, with no articles listed in the last 6 years.
Warning: This is likely a duplicate object, which shares a large percentage of members with at least one previously reported entry.
Warning: contains less than 25 stars with P>0.5 estimated.
Warning: the low UTI value and no obvious signs of duplication (C_dup=0.24) indicates that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Bica et al. (2019) | 283.473 | 0.627 | – | – | – | – |
| UCC | 283.421 | 0.608 | 0.173 | -1.985 | -4.485 | 56.565 |
Estimated members
Explore data in Colab
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| MCM 13 | 76.0 | 283.42 | 0.62 | 0.16 | -2.02 | -4.45 | 56.56 | 0.08 |