HSC 2499
Summary
HSC 2499 is a sparse, 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: 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) | 181.523 | -70.092 | 1.106 | -8.298 | -1.135 | -3.694 |
| Cavallo et al. (2024) | 182.007 | -70.199 | 1.102 | – | – | – |
| UCC | 181.827 | -70.102 | 1.1 | -8.19 | -1.142 | -2.133 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=0.566, diffAV50=0.306, MOD50=9.691, logAge50=8.487 |
| Cavallo et al. (2024) | AV50=0.75, dMod50=9.84, logAge50=8.49, [Fe/H]50=0.48 |
Search coordinates in Bayestar19
