HSC 1018
Summary
HSC 1018 is a poorly populated, very loose object of intermediate C3 quality. It is located at a large distance from the Sun, above the mid-plane. It was recently reported in the literature.
This object shares a large percentage of members with a later reported entry.
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) | 23.339 | 66.918 | 0.146 | -1.594 | 0.355 | – |
| Hunt & Reffert (2024) | 23.339 | 66.918 | 0.146 | -1.594 | 0.355 | – |
| UCC | 23.269 | 66.914 | 0.147 | -1.565 | 0.351 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=2.714, diffAV50=1.211, MOD50=13.882, logAge50=7.868 |
| Hunt & Reffert (2024) | MassJ=267.973, MassTot=442.283 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| CWNU 4737 | 88.0 | 23.24 | 66.91 | 0.16 | -1.55 | 0.35 | – | 0.08 |
