NGC 2143
(MWSC 711)
0.16
UTI
0.0
CN
0.03
Cdens
0.12
CC3
0.32
Clit
1.0
Cdup
Nm (P>50%)
22
Core radius and density
3.9 [pc], 0.1 [pc-2]
- CN 0.0 Sparse
- Cdens 0.03 Very loose
- CC3 0.12 Very low quality
- Clit 0.32 Poorly studied
- Cdup 1.0 Unique
Overview
NGC 2143 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a moderate* distance, below the mid-plane, affected by low extinction. It is catalogued as an old cluster (see Parameters). It is poorly studied in the literature.
(*): The parallax distance estimate (~3.29 kpc) differs significantly from the median photometric distance (~1.49 kpc).
â ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 90.737 | 5.769 | 0.304 | -0.466 | -0.167 | 55.542 |
| Just et al. | 2023 | 90.793 | 5.746 | â | â | â | â |
| Bica et al. | 2019 | 90.756 | 5.722 | â | â | â | â |
| Dias et al. | 2018 | â | â | â | 1.05 | -1.82 | â |
| Dib et al. | 2018 | 90.799 | 5.745 | â | â | â | â |
| Loktin & Popova | 2017 | 90.795 | 5.746 | â | -0.245 | -0.591 | â |
| Sampedro et al. | 2017 | 90.779 | 5.728 | â | 1.21 | -4.37 | â |
| Joshi et al. | 2016 | 90.799 | 5.745 | â | â | â | â |
| Kharchenko et al. | 2016 | 90.793 | 5.746 | â | â | â | â |
| Dias et al. | 2014 | 90.779 | 5.728 | â | 1.26 | -3.43 | â |
| Kharchenko et al. | 2013 | 90.799 | 5.745 | â | -1.37 | -1.69 | â |
| Piskunov et al. | 2008 | 90.773 | 5.776 | â | â | â | â |
| Kharchenko et al. | 2005 | 90.78 | 5.77 | â | 2.85 | 2.4 | â |
đĄ Note: The UCC values are estimated from its identified members.
| Reference | Year | Dist [kpc] | Av [mag] | DAv [mag] | Age [Myr] | [Fe/H] [dex] | Mass [Msun] | Bfrac | BSS |
|---|---|---|---|---|---|---|---|---|---|
| UCC | 99999â | 1.49 | 0.885 | â | 1230 | â | 226 | â | â |
| Just et al. | 2023 | â | â | â | 1230 | â | 374 | â | â |
| Dib et al. | 2018 | 1.49 | â | â | 1230 | â | â | â | â |
| Loktin & Popova | 2017 | 0.86 | 0.46 | â | 832 | â | â | â | â |
| Joshi et al. | 2016 | 1.49 | 1.31 | â | 1230 | â | 79 | â | â |
| Kharchenko et al. | 2016 | 1.49 | 1.31 | â | 1230 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.49 | 1.31 | â | 1230 | â | â | â | â |
| Piskunov et al. | 2008 | 0.80 | 0.00 | â | 1413 | â | â | â | â |
| Kharchenko et al. | 2005 | 0.80 | 0.00 | â | 1413 | â | â | â | â |
MOCA
