ADS 16795
(AR Cas)
Summary
ADS 16795 is a poorly populated, very loose object of low C3 quality. It is located at a very close distance from the Sun, near the mid-plane. It is poorly studied in the literature.
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 |
|---|---|---|---|---|---|---|
| Bica et al. (2019) | 352.517 | 58.549 | – | – | – | – |
| Hunt & Reffert (2023) | 352.592 | 58.553 | 4.76 | 18.657 | 2.847 | -13.358 |
| Cavallo et al. (2024) | 348.653 | 57.265 | 4.778 | – | – | – |
| UCC | 351.39 | 58.442 | 4.421 | 19.163 | 2.168 | -12.682 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=0.174, diffAV50=0.471, MOD50=6.65, logAge50=7.755 |
| Cavallo et al. (2024) | AV50=0.77, dMod50=6.67, logAge50=7.54, [Fe/H]50=-0.07 |
Search coordinates in Bayestar19
