HSC 1455
Summary
HSC 1455 is a sparse, very loose object of low C3 quality. It is located at a relatively close 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) | 92.259 | 27.199 | 0.653 | -1.194 | -4.719 | – |
| Cavallo et al. (2024) | 92.288 | 27.143 | 0.652 | – | – | – |
| Hunt & Reffert (2024) | 92.259 | 27.199 | 0.653 | -1.194 | -4.719 | – |
| UCC | 92.291 | 27.173 | 0.64 | -1.192 | -4.731 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=0.803, diffAV50=0.59, MOD50=10.806, logAge50=8.444 |
| Cavallo et al. (2024) | AV50=1.21, dMod50=11.01, logAge50=8.3, [Fe/H]50=-0.22 |
| Hunt & Reffert (2024) | MassJ=51.0126, MassTot=105.337 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| CWNU 4136 | 96.0 | 92.29 | 27.17 | 0.64 | -1.19 | -4.7 | – | 0.0 |
