HSC 2490
Summary
HSC 2490 is a poorly populated, very loose object of intermediate C3 quality. It is located at a 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) | 180.684 | -68.588 | 1.043 | -5.32 | -1.043 | 12.271 |
| Cavallo et al. (2024) | 178.491 | -68.545 | 1.042 | – | – | – |
| UCC | 178.115 | -68.448 | 1.04 | -5.323 | -1.013 | 10.707 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=0.445, diffAV50=0.814, MOD50=9.806, logAge50=8.391 |
| Cavallo et al. (2024) | AV50=0.85, dMod50=9.88, logAge50=8.45, [Fe/H]50=0.04 |
Search coordinates in Bayestar19
