Collinder 144
(NGC 2395; OCL 502; MWSC 1228)
Summary
Collinder 144 is a sparse, very loose object of very low C3 quality. It is located at a very large distance from the Sun, well above 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 |
|---|---|---|---|---|---|---|
| Dias et al. (2002) | 111.8 | 13.608 | – | -3.36 | -6.02 | – |
| Loktin & Popova (2017) | 111.795 | 13.608 | – | -2.109 | -5.187 | – |
| Bica et al. (2019) | 111.776 | 13.592 | – | – | – | – |
| UCC | 111.755 | 13.593 | 0.054 | -0.386 | -0.895 | 48.734 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2002) | E(B-V)=0.12, Dist=512.0, Age=9.07 |
| Loktin & Popova (2017) | E(B-V)=0.119, Dist=592, logt=9.072 |
Search coordinates in Bayestar19