HSC 2050
Summary
HSC 2050 is a sparse, very loose object of intermediate 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) | 128.049 | -36.112 | 0.914 | -5.051 | 4.525 | 20.495 |
| Cavallo et al. (2024) | 128.044 | -36.279 | 0.911 | – | – | – |
| Hunt & Reffert (2024) | 128.049 | -36.112 | 0.914 | -5.051 | 4.525 | 20.495 |
| UCC | 128.085 | -36.341 | 0.911 | -5.018 | 4.545 | 27.823 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=0.487, diffAV50=0.331, MOD50=10.111, logAge50=7.591 |
| Cavallo et al. (2024) | AV50=0.52, dMod50=10.28, logAge50=7.67, [Fe/H]50=0.59 |
| Hunt & Reffert (2024) | MassJ=67.7576, MassTot=72.3254 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| CWNU 4709 | 80.0 | 127.91 | -36.29 | 0.91 | -5.02 | 4.56 | 21.05 | 0.03 |
