Pismis 14
(OCL 780; ESO 166 16; MWSC 1678)
Summary
Pismis 14 is a sparse, very loose object of very low C3 quality. It is located at a moderate distance from the Sun, below the mid-plane. It is poorly studied in the literature, with no articles listed in the last 6 years.
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) | 142.463 | -52.783 | – | -3.69 | 4.79 | – |
| Kharchenko et al. (2012) | 142.47 | -52.78 | – | -6.65 | 4.71 | – |
| Bica et al. (2019) | 142.456 | -52.773 | – | – | – | – |
| UCC | 142.458 | -52.797 | 0.235 | -4.545 | 2.728 | 61.818 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2002) | E(B-V)=0.56, Dist=1314.0, Age=7.35 |
| Kharchenko et al. (2012) | e_bv=0.479, distance=1775, log_age=8.355 |
Search coordinates in Bayestar19