MWSC 4349
Summary
MWSC 4349 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) | 261.757 | -57.525 | – | -3.52 | -7.65 | – |
| Bica et al. (2019) | 261.76 | -57.529 | – | – | – | – |
| UCC | 261.693 | -57.531 | 0.176 | -2.267 | -4.013 | 30.786 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Kharchenko et al. (2012) | e_bv=0.521, distance=3210, log_age=8.805 |
Search coordinates in Bayestar19