HSC 2399
Summary
HSC 2399 is a poorly populated, loose object of low C3 quality. It is located at a very close distance from the Sun, near the mid-plane. It was recently reported in the literature.This is a unique object, which shares a very small percentage of members with at least one previously reported entry.
Warning: the low UTI value and no obvious signs of duplication (C_dup=0.96) 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) | 142.232 | -73.779 | 12.706 | -30.657 | 33.088 | 16.192 |
| Cavallo et al. (2024) | 140.612 | -72.984 | 12.706 | – | – | – |
| UCC | 147.135 | -73.681 | 12.799 | -31.554 | 34.243 | 15.309 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=1.182, diffAV50=1.167, MOD50=4.424, logAge50=8.203 |
| Cavallo et al. (2024) | AV50=0.75, dMod50=4.52, logAge50=7.49, [Fe/H]50=-0.29 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| OCSN 88 | 3.8 | 141.23 | -64.97 | 11.27 | -32.0 | 41.95 | 23.59 | 0.46 |
