HSC 381
Summary
HSC 381 is a poorly populated, very loose object of high C3 quality. It is located at a very close distance from the Sun, above the mid-plane. It was recently reported in the literature.This is a unique object, which shares a very small percentage of members with at least one previously reported entry.
Warning: the low UTI value and no obvious signs of duplication (C_dup=0.96) 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 |
|---|---|---|---|---|---|---|
| Hunt & Reffert (2023) | 271.386 | 17.771 | 3.161 | -1.036 | -8.11 | -17.045 |
| Cavallo et al. (2024) | 270.773 | 19.135 | 3.178 | – | – | – |
| UCC | 270.961 | 19.467 | 3.227 | -1.162 | -8.033 | -16.73 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=0.211, diffAV50=0.827, MOD50=7.464, logAge50=7.487 |
| Cavallo et al. (2024) | AV50=0.66, dMod50=7.53, logAge50=7.22, [Fe/H]50=-0.05 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| OCSN 11 | 3.7 | 270.09 | 21.47 | 3.39 | -1.34 | -7.63 | -18.06 | 0.19 |
