HSC 1749
Summary
HSC 1749 is a poorly populated, very loose object of low C3 quality. It is located at a moderate distance from the Sun, below the mid-plane. It was recently reported 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 |
|---|---|---|---|---|---|---|
| Hunt & Reffert (2023) | 105.141 | -9.027 | 0.363 | -1.883 | 2.23 | – |
| Cavallo et al. (2024) | 105.114 | -8.9 | 0.361 | – | – | – |
| UCC | 105.135 | -9.031 | 0.349 | -1.901 | 2.267 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=1.206, diffAV50=1.598, MOD50=11.952, logAge50=8.027 |
| Cavallo et al. (2024) | AV50=0.74, dMod50=12.43, logAge50=8.3, [Fe/H]50=0.35 |
Search coordinates in Bayestar19
