HSC 2409
Summary
HSC 2409 is a sparse, very loose object of low C3 quality. It is located at a large distance from the Sun, well below the mid-plane. It was recently reported in the literature.
This object shares a small percentage of members with a later 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=1.0) 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) | 163.541 | -65.671 | 0.138 | -5.584 | 2.499 | 51.174 |
| Hunt & Reffert (2024) | 163.541 | -65.671 | 0.138 | -5.584 | 2.499 | 51.174 |
| UCC | 163.544 | -65.659 | 0.139 | -5.56 | 2.483 | 51.293 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=1.348, diffAV50=1.249, MOD50=13.937, logAge50=9.633 |
| Hunt & Reffert (2024) | MassJ=942.026, MassTot=1383.68 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| CWNU 4861 | 12.0 | 163.36 | -65.54 | 0.18 | -5.83 | 2.42 | 24.13 | 0.03 |
