HSC 1655
Summary
HSC 1655 is a sparse, loose object of low C3 quality. It is located at a moderate distance from the Sun, below the mid-plane. It was recently reported in the literature.
This object shares a large 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) | 99.793 | 1.773 | 0.245 | 0.347 | -1.006 | 31.83 |
| Hunt & Reffert (2024) | 99.793 | 1.773 | 0.245 | 0.347 | -1.006 | 31.83 |
| UCC | 99.742 | 1.798 | 0.252 | 0.354 | -1.069 | 29.822 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=2.649, diffAV50=1.397, MOD50=12.711, logAge50=8.88 |
| Hunt & Reffert (2024) | MassJ=267.384, MassTot=285.186 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| CWNU 3581 | 88.0 | 99.72 | 1.8 | 0.25 | 0.35 | -1.08 | 29.82 | 0.06 |
