Basel 14
(MWSC 3498)
Summary
Basel 14 is a sparse, very loose object of low C3 quality. It is located at a moderate distance from the Sun, below the mid-plane. It is poorly studied 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 |
|---|---|---|---|---|---|---|
| Dias et al. (2002) | 320.325 | 44.817 | – | -1.85 | 0.81 | – |
| Kharchenko et al. (2013) | 320.257 | 44.825 | – | -3.81 | -3.5 | – |
| Kharchenko et al. (2016) | 320.252 | 44.822 | – | – | – | – |
| Loktin & Popova (2017) | 320.25 | 44.821 | – | -2.13 | -1.917 | – |
| Just et al. (2023) | 320.252 | 44.822 | – | – | – | – |
| UCC | 320.269 | 44.786 | 0.205 | -3.81 | -3.269 | -43.917 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2002) | E(B-V)=0.65, Dist=964.0, Age=8.3 |
| Kharchenko et al. (2013) | E(B-V)=0.687, d=1802.0, logt=8.805 |
| Kharchenko et al. (2016) | E(B-V)=0.687, d=1802.0, logt=8.805 |
| Loktin & Popova (2017) | E(B-V)=0.309, Dist=1754, logt=8.98 |
| Just et al. (2023) | logt=8.805, logmt=1.902 |
Search coordinates in Bayestar19