Collinder 333
(MWSC 2618; OCL 1017; ESO 393 04)
0.69
UTI
0.43
CN
1.0
Cdens
0.75
CC3
0.62
Clit
1.0
Cdup
Stellar density (N50/rad)
5.5 [N/pc2]
- CN 0.43 Poorly populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.62 Moderately studied
- Cdup 1.0 Unique
Overview
Collinder 333 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a moderate* distance, near the mid-plane, affected by high extinction. It is catalogued as a very metal-poor, intermediate-age cluster, but with a large variance across recent sources for the age and mass parameters (see Parameters). It is moderately studied in the literature.
(*): The parallax distance estimate (~2.59 kpc) differs significantly from the median photometric distance (~1.05 kpc).
Note: This object shares a significant percentage of members with a later reported entry. See table with shared members information.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 262.85 | -34.003 | 0.386 | 0.055 | -1.092 | -23.739 |
| Hunt & Reffert | 2024 | 262.788 | -33.998 | 0.398 | 0.023 | -1.103 | 64.058 |
| Cavallo et al. | 2024 | 262.822 | -33.999 | 0.397 | â | â | â |
| Hunt & Reffert | 2023 | 262.788 | -33.998 | 0.398 | 0.023 | -1.103 | 64.058 |
| Just et al. | 2023 | 262.895 | -34.01 | â | â | â | â |
| Bica et al. | 2019 | 262.869 | -34.023 | â | â | â | â |
| Kharchenko et al. | 2016 | 262.895 | -34.01 | â | â | â | â |
| Dias et al. | 2014 | 262.879 | -34.017 | â | -2.42 | 0.38 | â |
| Kharchenko et al. | 2013 | 262.905 | -34.01 | â | 0.71 | -2.25 | â |
| Piskunov et al. | 2008 | 262.869 | -34.023 | â | â | â | â |
| Kharchenko et al. | 2005 | 262.87 | -34.02 | â | 0.68 | -4.88 | â |
| Dias et al. | 2002 | 262.879 | -34.017 | â | -2.42 | 0.38 | 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 | 1.05 | 3.29 | 3.02 | 141 | -1.640 | 688 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 1348(1) | â | â |
| Cavallo et al. | 2024 | 1.39 | 5.34 | â | 1 | -1.640 | â | â | â |
| Hunt & Reffert | 2023 | 2.34 | 4.70 | 3.02 | 5 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 141 | â | 27 | â | â |
| Kharchenko et al. | 2016 | 1.05 | 3.29 | â | 141 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.05 | 3.29 | â | 141 | â | â | â | â |
| Piskunov et al. | 2008 | 0.85 | 0.34 | â | 794 | â | â | â | â |
| Kharchenko et al. | 2005 | 0.85 | 0.34 | â | 794 | â | â | â | â |
| Dias et al. | 2002 | 0.85 | 0.34 | â | 794 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Cavallo et al. (2024)
Wood sample.