HSC 1689
Summary
HSC 1689 is a sparse, very loose object of low C3 quality. It is located at a large 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) | 101.503 | -1.951 | 0.129 | -0.325 | 0.329 | – |
| Hunt & Reffert (2024) | 101.503 | -1.951 | 0.129 | -0.325 | 0.329 | – |
| UCC | 101.499 | -1.96 | 0.127 | -0.332 | 0.315 | 111.595 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=3.3, diffAV50=2.064, MOD50=13.993, logAge50=7.551 |
| Hunt & Reffert (2024) | MassJ=1323.93, MassTot=1323.93 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| CWNU 3261 | 88.0 | 101.5 | -1.97 | 0.11 | -0.33 | 0.31 | 111.59 | 0.01 |
