HSC 1751
Summary
HSC 1751 is a poorly populated, very loose object of low C3 quality. It is located at a very close distance from the Sun, below the mid-plane. It was recently reported in the literature.
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) | 96.276 | -13.469 | 2.78 | -4.952 | 1.104 | 17.933 |
| UCC | 95.89 | -13.538 | 2.769 | -4.921 | 1.164 | 16.625 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=0.06, diffAV50=0.322, MOD50=7.69, logAge50=8.041 |
Search coordinates in Bayestar19
