MWSC 4408
Summary
MWSC 4408 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) | 273.877 | -60.215 | – | -1.6 | -7.99 | – |
| Bica et al. (2019) | 273.88 | -60.212 | – | – | – | – |
| UCC | 273.794 | -60.153 | 0.453 | -3.352 | -7.721 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Kharchenko et al. (2012) | e_bv=0.687, distance=2167, log_age=8.495 |
Search coordinates in Bayestar19