HSC 1469
Summary
HSC 1469 is a poorly populated, very loose object of high 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) | 48.175 | -4.372 | 5.585 | 2.352 | -6.067 | 9.221 |
| Cavallo et al. (2024) | 51.707 | -4.167 | 5.566 | – | – | – |
| UCC | 51.734 | -4.599 | 5.553 | 2.526 | -6.175 | 9.488 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=0.311, diffAV50=0.821, MOD50=6.272, logAge50=8.292 |
| Cavallo et al. (2024) | AV50=0.65, dMod50=6.21, logAge50=7.5, [Fe/H]50=0.11 |
Search coordinates in Bayestar19
