HSC 2275
Summary
HSC 2275 is a sparse, loose object of intermediate 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) | 146.942 | -56.458 | 0.196 | -4.852 | 3.519 | – |
| Hunt & Reffert (2024) | 146.942 | -56.458 | 0.196 | -4.852 | 3.519 | – |
| UCC | 146.931 | -56.463 | 0.193 | -4.848 | 3.504 | 41.19 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=3.133, diffAV50=0.385, MOD50=13.518, logAge50=8.478 |
| Hunt & Reffert (2024) | MassJ=530.815, MassTot=414.239 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| CWNU 3735 | 88.0 | 146.93 | -56.46 | 0.19 | -4.85 | 3.5 | 41.19 | 0.02 |
