HSC 1365
Summary
HSC 1365 is a sparse, 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: 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) | 88.29 | 36.124 | 0.213 | -0.219 | -0.848 | – |
| Cavallo et al. (2024) | 88.35 | 36.169 | 0.211 | – | – | – |
| UCC | 88.336 | 36.139 | 0.188 | -0.237 | -0.851 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=1.415, diffAV50=0.972, MOD50=13.321, logAge50=7.678 |
| Cavallo et al. (2024) | AV50=1.22, dMod50=13.16, logAge50=7.54, [Fe/H]50=-0.06 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| CWNU 3517 | 92.0 | 88.34 | 36.14 | 0.18 | -0.19 | -0.85 | – | 0.07 |
