HSC 2511
Summary
HSC 2511 is a sparse, very loose object of intermediate C3 quality. It is located at a close distance from the Sun, above 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) | 186.827 | -58.34 | 1.105 | -10.233 | -2.229 | -11.078 |
| Cavallo et al. (2024) | 186.942 | -58.569 | 1.108 | – | – | – |
| UCC | 187.055 | -58.385 | 1.102 | -10.17 | -2.201 | -15.657 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=0.203, diffAV50=0.597, MOD50=9.701, logAge50=8.608 |
| Cavallo et al. (2024) | AV50=0.95, dMod50=9.71, logAge50=8.01, [Fe/H]50=-0.09 |
Search coordinates in Bayestar19
