MWSC 4409
Summary
MWSC 4409 is a poorly populated, 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: 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) | 273.84 | 31.725 | – | 0.29 | -4.72 | – |
| Bica et al. (2019) | 273.834 | 31.725 | – | – | – | – |
| UCC | 273.855 | 31.725 | 0.214 | -2.317 | -3.422 | -114.591 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Kharchenko et al. (2012) | e_bv=0.656, distance=2740, log_age=8.85 |
Search coordinates in Bayestar19