HSC 2582
Summary
HSC 2582 is a sparse, very loose object of high C3 quality. It is located at a moderate 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: contains less than 25 stars with P>0.5 estimated.
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) | 200.757 | -61.156 | 0.451 | -3.657 | -1.734 | – |
| Hunt & Reffert (2024) | 200.757 | -61.156 | 0.451 | -3.657 | -1.734 | – |
| UCC | 200.782 | -61.163 | 0.45 | -3.659 | -1.732 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=0.851, diffAV50=0.459, MOD50=11.662, logAge50=8.173 |
| Hunt & Reffert (2024) | MassJ=140.935, MassTot=146.114 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| UBC 292 | 4.0 | 200.17 | -61.31 | 0.43 | -3.65 | -1.65 | – | 0.47 |
