HSC 444
Summary
HSC 444 is a poorly populated, loose object of high C3 quality. It is located at a moderate distance from the Sun, below the mid-plane. It was recently reported in the literature.
This object shares a large percentage of members with a later reported entry.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Hunt & Reffert (2023) | 295.127 | 17.785 | 0.307 | -1.988 | -2.568 | 38.05 |
| Cavallo et al. (2024) | 295.102 | 17.793 | 0.303 | – | – | – |
| Hunt & Reffert (2024) | 295.127 | 17.785 | 0.307 | -1.988 | -2.568 | 38.05 |
| UCC | 295.097 | 17.777 | 0.289 | -1.97 | -2.554 | 19.436 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=2.684, diffAV50=2.273, MOD50=12.418, logAge50=7.88 |
| Cavallo et al. (2024) | AV50=2.55, dMod50=12.57, logAge50=8.23, [Fe/H]50=0.6 |
| Hunt & Reffert (2024) | MassJ=396.821, MassTot=586.489 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| CWNU 3408 | 96.3 | 295.1 | 17.78 | 0.29 | -1.98 | -2.55 | 19.44 | 0.03 |
