HSC 2100
Summary
HSC 2100 is a sparse, very loose object of low C3 quality. It is located at a very large distance from the Sun, well 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) | 124.693 | -44.733 | 0.075 | -1.755 | 2.63 | – |
| Hunt & Reffert (2024) | 124.693 | -44.733 | 0.075 | -1.755 | 2.63 | – |
| UCC | 124.697 | -44.737 | 0.083 | -1.73 | 2.615 | 104.497 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=2.694, diffAV50=1.202, MOD50=15.347, logAge50=8.69 |
| Hunt & Reffert (2024) | MassJ=1942.23, MassTot=1942.23 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| CWNU 3636 | 80.0 | 124.7 | -44.74 | 0.08 | -1.75 | 2.56 | 107.34 | 0.03 |
