HSC 1622
Summary
HSC 1622 is a sparse, very loose object of low C3 quality. It is located at a relatively close distance from the Sun, near 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) | 99.567 | 6.161 | 0.76 | 0.261 | -3.666 | 31.753 |
| Cavallo et al. (2024) | 99.526 | 6.116 | 0.76 | – | – | – |
| Hunt & Reffert (2024) | 99.567 | 6.161 | 0.76 | 0.261 | -3.666 | 31.753 |
| UCC | 99.547 | 6.136 | 0.761 | 0.252 | -3.678 | 20.908 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=0.645, diffAV50=0.799, MOD50=10.418, logAge50=8.201 |
| Cavallo et al. (2024) | AV50=0.73, dMod50=10.59, logAge50=8.35, [Fe/H]50=0.29 |
| Hunt & Reffert (2024) | MassJ=44.9808, MassTot=92.4575 |
Search coordinates in Bayestar19