MWSC 4287
Summary
MWSC 4287 is a sparse, very loose object of very low C3 quality. It is located at a large 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) | 250.65 | -24.46 | – | -4.53 | -5.69 | – |
| Bica et al. (2019) | 250.653 | -24.462 | – | – | – | – |
| UCC | 250.668 | -24.459 | 0.165 | -3.832 | -5.374 | 50.665 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Kharchenko et al. (2012) | e_bv=1.832, distance=2524, log_age=7.92 |
Search coordinates in Bayestar19