HSC 2687
Summary
HSC 2687 is a poorly populated, loose object of intermediate C3 quality. It is located at a very close distance from the Sun, near 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) | 225.209 | -54.445 | 2.433 | -7.636 | -8.73 | -10.29 |
| Cavallo et al. (2024) | 224.988 | -54.588 | 2.423 | – | – | – |
| UCC | 225.048 | -54.48 | 2.437 | -7.659 | -8.635 | -10.347 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=0.334, diffAV50=0.649, MOD50=7.998, logAge50=7.566 |
| Cavallo et al. (2024) | AV50=0.74, dMod50=8.18, logAge50=7.4, [Fe/H]50=0.43 |
Search coordinates in Bayestar19
