Collinder 223
(MWSC 1815)
0.35
UTI
0.0
CN
0.08
Cdens
0.12
CC3
0.78
Clit
1.0
Cdup
Stellar density (N50/rad)
0.4 [N/pc2]
- CN 0.0 Sparse
- Cdens 0.08 Very loose
- CC3 0.12 Very low quality
- Clit 0.78 Well-studied
- Cdup 1.0 Unique
Overview
Collinder 223 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 a near-solar metallicity, intermediate-age cluster (see Parameters). It is well-studied in the literature.
(*): The parallax distance estimate (~3.72 kpc) differs significantly from the median photometric distance (~1.69 kpc).
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 157.937 | -59.941 | 0.269 | -6.964 | 3.63 | -19.242 |
| Just et al. | 2023 | 157.637 | -59.851 | â | â | â | â |
| Jaehnig et al. | 2021 | 157.786 | -60.05 | 0.411 | -5.423 | 2.859 | â |
| Loktin & Popova | 2017 | 158.07 | -60.02 | â | -5.32 | -2.46 | 8.5 |
| Kharchenko et al. | 2016 | 157.637 | -59.851 | â | â | â | â |
| Dias et al. | 2014 | 158.067 | -60.02 | â | -5.32 | -2.46 | â |
| Kharchenko et al. | 2013 | 157.642 | -59.855 | â | -7.56 | 2.25 | 8.5 |
| Gozha et al. | 2012 | 158.067 | -60.02 | â | â | â | â |
| Piskunov et al. | 2008 | 157.596 | -59.816 | â | â | â | â |
| Kharchenko et al. | 2007 | 158.07 | -60.02 | â | 0.15 | â | 4.7 |
| van den Bergh | 2006 | 157.6 | -59.817 | â | â | â | â |
| Kharchenko et al. | 2005 | 157.59 | -59.82 | â | -7.17 | 1.08 | 4.7 |
| Kharchenko et al. | 2003 | 157.57 | -59.82 | â | -7.89 | 1.26 | â |
| Dias et al. | 2002 | 158.067 | -60.02 | â | -5.32 | -2.46 | 2.0 |
| Dambis | 1999 | 158.067 | -60.02 | â | â | â | 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 | 1.69 | 0.76 | â | 129 | -0.217 | 416 | â | â |
| Just et al. | 2023 | â | â | â | 158 | â | 38 | â | â |
| Jaehnig et al. | 2021 | 2.61(1) | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 1.69 | 0.54 | â | 60 | â | â | â | â |
| Kharchenko et al. | 2016 | 1.38 | 1.03 | â | 158 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.38 | 1.03 | â | 158 | -0.217 | â | â | â |
| Gozha et al. | 2012 | 2.82 | â | â | 100 | â | 794 | â | â |
| Piskunov et al. | 2008 | 1.69 | 0.56 | â | 257 | â | â | â | â |
| van den Bergh | 2006 | 1.69 | 0.81 | â | 10 | â | â | â | â |
| Kharchenko et al. | 2005 | 1.69 | 0.56 | â | 257 | â | â | â | â |
| Kharchenko et al. | 2003 | 1.69 | 0.56 | â | â | â | â | â | â |
| Dias et al. | 2002 | 2.82 | 0.78 | â | 100 | -0.217 | â | â | â |
| Dambis | 1999 | 2.14 | 0.76 | â | 79 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA
