LS 474
(La Serena 474)
Summary
LS 474 is a rich, very dense object of very low C3 quality. It is located at a relatively close distance from the Sun, near the mid-plane. It is rarely studied in the literature, with no articles listed in the last 6 years.
This is very likely a unique object, which shares a small percentage of members with at least one previously reported entry, and a very small percentage with at least one entry reported in the same catalogue.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Bica et al. (2019) | 257.904 | -38.354 | – | – | – | – |
| UCC | 257.881 | -38.296 | 0.584 | -2.455 | -3.32 | -27.477 |
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 |
|---|---|---|---|---|---|---|---|---|
| FSR 1755 | 15.3 | 258.1 | -38.44 | 0.61 | -2.63 | -3.64 | -36.13 | 0.18 |
| Teutsch 258 | 3.2 | 257.85 | -38.43 | 0.64 | -2.81 | -4.64 | -34.03 | 0.09 |
| Ryu 401 | 1.3 | 257.95 | -38.61 | 0.66 | -1.41 | -3.07 | -39.66 | 0.23 |