MWSC 5627
Summary
MWSC 5627 is a sparse, very loose object of low C3 quality. It is located at a large 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) | 64.793 | 20.335 | – | 1.56 | -7.0 | – |
| Bica et al. (2019) | 64.779 | 20.334 | – | – | – | – |
| UCC | 64.809 | 20.339 | 0.184 | 0.103 | -1.083 | -66.457 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Kharchenko et al. (2012) | e_bv=0.312, distance=1659, log_age=9.25 |
Search coordinates in Bayestar19