HSC 1827
Summary
HSC 1827 is a sparse, very loose object of low C3 quality. It is located at a very close distance from the Sun, near the mid-plane. It was recently reported in the literature.
This is very likely a unique object, which shares a small percentage of members with at least one previously 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=0.84) 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) | 102.757 | -20.154 | 2.519 | -6.44 | 4.836 | 17.348 |
| UCC | 103.076 | -20.111 | 2.524 | -6.429 | 4.855 | 16.684 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=0.122, diffAV50=0.358, MOD50=7.922, logAge50=7.832 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| OCSN 78 | 16.0 | 100.45 | -19.49 | 2.69 | -6.26 | 5.16 | 22.32 | 0.31 |
