MWSC 4317
Summary
MWSC 4317 is a sparse, very loose object of low C3 quality. It is located at a moderate distance from the Sun, well above the mid-plane. It is rarely 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 |
|---|---|---|---|---|---|---|
| Kharchenko et al. (2012) | 257.618 | 1.265 | – | -2.07 | -0.16 | – |
| Bica et al. (2019) | 257.619 | 1.26 | – | – | – | – |
| UCC | 257.631 | 1.231 | 0.288 | -4.548 | -4.86 | 75.398 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Kharchenko et al. (2012) | e_bv=0.333, distance=2391, log_age=9.425 |
Search coordinates in Bayestar19