HSC 1450
Summary
HSC 1450 is a sparse, very loose object of low 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) | 88.995 | 25.716 | 0.194 | 0.298 | -0.652 | 54.41 |
| Cavallo et al. (2024) | 88.959 | 25.697 | 0.194 | – | – | – |
| Hunt & Reffert (2024) | 88.995 | 25.716 | 0.194 | 0.298 | -0.652 | 54.41 |
| UCC | 89.008 | 25.725 | 0.192 | 0.313 | -0.648 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=2.499, diffAV50=1.878, MOD50=13.256, logAge50=8.051 |
| Cavallo et al. (2024) | AV50=2.29, dMod50=13.07, logAge50=8.28, [Fe/H]50=0.63 |
| Hunt & Reffert (2024) | MassJ=771.462, MassTot=1037.64 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| CWNU 3842 | 88.0 | 88.99 | 25.72 | 0.19 | 0.29 | -0.63 | – | 0.04 |
