HSC 1665
Summary
HSC 1665 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) | 99.562 | 0.735 | 0.145 | -0.213 | 0.386 | 82.575 |
| Cavallo et al. (2024) | 99.634 | 0.757 | 0.148 | – | – | – |
| Hunt & Reffert (2024) | 99.562 | 0.735 | 0.145 | -0.213 | 0.386 | 82.575 |
| UCC | 99.606 | 0.743 | 0.142 | -0.251 | 0.367 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=2.695, diffAV50=2.381, MOD50=14.106, logAge50=7.284 |
| Cavallo et al. (2024) | AV50=2.36, dMod50=13.06, logAge50=7.64, [Fe/H]50=0.08 |
| Hunt & Reffert (2024) | MassJ=1023.11, MassTot=1144.96 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| CWNU 3647 | 96.0 | 99.64 | 0.76 | 0.15 | -0.21 | 0.38 | 82.57 | 0.33 |
