NGC 2306
(MWSC 1014)
Summary
NGC 2306 is a sparse, very loose object of very low C3 quality. It is located at a moderate distance from the Sun, below the mid-plane. It is poorly 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 |
|---|---|---|---|---|---|---|
| Piskunov et al. (2008) | 103.61 | -7.217 | – | – | – | – |
| Loktin & Popova (2017) | 103.605 | -7.202 | – | 0.923 | -0.736 | – |
| Bica et al. (2019) | 103.646 | -7.176 | – | – | – | – |
| UCC | 103.607 | -7.185 | 0.203 | 0.066 | 0.625 | 87.289 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Piskunov et al. (2008) | E(B-V)=0.05, Dist=1200, logt=8.85, logMA=2.147 |
| Loktin & Popova (2017) | E(B-V)=0.235, Dist=2189, logt=9.07 |
Search coordinates in Bayestar19