HSC 1426
Summary
HSC 1426 is a poorly populated, very dense object of very high C3 quality. It is located at a very close distance from the Sun, below the mid-plane. It was recently reported in the literature.
Warning: This is likely a duplicate object, which shares a large percentage of members with at least one previously reported entry.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Hunt & Reffert (2023) | 56.478 | 5.943 | 5.345 | 20.251 | -12.985 | 16.457 |
| Cavallo et al. (2024) | 58.235 | 5.2 | 5.397 | – | – | – |
| UCC | 56.523 | 6.051 | 5.463 | 21.204 | -13.456 | 16.793 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=0.121, diffAV50=0.339, MOD50=6.334, logAge50=7.902 |
| Cavallo et al. (2024) | AV50=0.93, dMod50=6.39, logAge50=7.69, [Fe/H]50=0.06 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| UPK 378 | 80.0 | 56.43 | 6.05 | 5.5 | 21.5 | -13.58 | 16.2 | 0.4 |
