MWSC 4484
Summary
MWSC 4484 is a poorly populated, very loose object of very low C3 quality. It is located at a moderate distance from the Sun, well below the mid-plane. It is rarely studied in the literature, with no articles listed in the last 6 years.
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) | 290.58 | -25.01 | – | 0.5 | -5.19 | – |
| Bica et al. (2019) | 290.582 | -25.017 | – | – | – | – |
| UCC | 290.598 | -25.027 | 0.246 | -4.225 | -5.498 | 1.23 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Kharchenko et al. (2012) | e_bv=0.437, distance=1667, log_age=9.045 |
Search coordinates in Bayestar19