Collinder 213
(MWSC 1725; OCL 785; ESO 213 04)
0.63
UTI
0.54
CN
0.58
Cdens
0.75
CC3
0.65
Clit
1.0
Cdup
Radius (P>50% members)
6.4 [arcmin]
- CN 0.54 Moderately populated
- Cdens 0.58 Moderately dense
- CC3 0.75 High quality
- Clit 0.65 Moderately studied
- Cdup 1.0 Unique
Overview
Collinder 213 is a moderately populated, moderately dense object of high C3 quality. Its parallax locates it at a moderate* distance, above the mid-plane, affected by low extinction. It is catalogued as a metal-rich, intermediate-age cluster (see Parameters). It is moderately studied in the literature.
(*): The parallax distance estimate (~2.40 kpc) differs significantly from the median photometric distance (~1.46 kpc).
Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.
Relatively close
Low extinction
Metal-rich
Intermediate age
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 148.693 | -50.916 | 0.416 | -6.854 | 5.054 | 11.126 |
| Hunt & Reffert | 2024 | 148.632 | -50.898 | 0.407 | -6.859 | 5.061 | 9.069 |
| Cavallo et al. | 2024 | 148.672 | -50.882 | 0.411 | â | â | â |
| Hunt & Reffert | 2023 | 148.632 | -50.898 | 0.407 | -6.859 | 5.061 | 9.069 |
| Just et al. | 2023 | 148.675 | -50.922 | â | â | â | â |
| Bica et al. | 2019 | 148.699 | -50.973 | â | â | â | â |
| Kharchenko et al. | 2016 | 148.675 | -50.922 | â | â | â | â |
| Dias et al. | 2014 | 148.679 | -50.917 | â | -3.66 | 2.48 | â |
| Kharchenko et al. | 2013 | 148.68 | -50.925 | â | -5.2 | 4.55 | â |
| Piskunov et al. | 2008 | 148.644 | -50.92 | â | â | â | â |
| Kharchenko et al. | 2005 | 148.65 | -50.92 | â | -3.96 | 2.58 | â |
| Dias et al. | 2002 | 148.679 | -50.917 | â | -3.66 | 2.48 | 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] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Hunt & Reffert | 2024 | â | â | â | â | â | 295* | â | â |
| Cavallo et al. | 2024 | 2.58 | 1.41 | â | 98 | 0.570 | â | â | â |
| Hunt & Reffert | 2023 | 2.18 | 1.18 | 1.19 | 191 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 741 | â | 202 | â | â |
| Kharchenko et al. | 2016 | 1.46 | 0.22 | â | 741 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.46 | 0.22 | â | 741 | â | â | â | â |
| Piskunov et al. | 2008 | 1.40 | 0.22 | â | 692 | â | â | â | â |
| Kharchenko et al. | 2005 | 1.40 | 0.22 | â | 692 | â | â | â | â |
| Dias et al. | 2002 | 1.40 | 0.22 | â | 692 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Gold sample.