NGC 2349
Summary
NGC 2349 is a sparse, very loose object of very low C3 quality. It is located at a moderate distance from the Sun, above the mid-plane. It is poorly studied in the literature, with no articles listed in the last 8 years.
This object shares a very small percentage of members with a later reported entry.
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 |
|---|---|---|---|---|---|---|
| Dias et al. (2002) | 107.7 | -8.593 | – | 0.71 | -2.23 | – |
| Kharchenko et al. (2012) | 107.677 | -8.605 | – | 2.6 | -3.28 | – |
| Loktin & Popova (2017) | 107.67 | -8.593 | – | -2.46 | -3.266 | – |
| UCC | 107.701 | -8.584 | 0.227 | -1.189 | 0.687 | 81.936 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2002) | E(B-V)=0.61, Dist=1628.0, Age=8.88 |
| Kharchenko et al. (2012) | e_bv=0.312, distance=1819, log_age=9.14 |
| Loktin & Popova (2017) | E(B-V)=0.211, Dist=4029, logt=9.18 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| Teutsch 171 | 4.0 | 107.84 | -8.4 | 0.34 | -1.2 | 1.01 | 82.55 | 0.1 |