MWSC 4606
Summary
MWSC 4606 is a sparse, very loose object of 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: 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) | 316.53 | -11.47 | – | 2.55 | -4.59 | – |
| Bica et al. (2019) | 316.532 | -11.473 | – | – | – | – |
| UCC | 316.551 | -11.508 | 0.225 | -1.96 | -6.232 | -83.228 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Kharchenko et al. (2012) | e_bv=0.271, distance=956, log_age=9.385 |
Search coordinates in Bayestar19