Collinder 228
0.79
UTI
0.62
CN
1.0
Cdens
0.75
CC3
0.78
Clit
1.0
Cdup
Stellar density (N50/rad)
11.5 [N/pc2]
- CN 0.62 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.78 Well-studied
- Cdup 1.0 Unique
Overview
Collinder 228 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by low extinction. It is catalogued as a massive, near-solar metallicity, very young cluster, but with a large variance across recent sources for the age parameter (see Parameters). It is well-studied in the literature.
Note: This object shares a moderate 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 | 161.009 | -60.09 | 0.399 | -6.698 | 1.921 | -11.487 |
| Hunt & Reffert | 2024 | 161.011 | -60.091 | 0.399 | -6.668 | 1.92 | -28.406 |
| Cavallo et al. | 2024 | 161.013 | -60.081 | 0.399 | â | â | â |
| Hunt & Reffert | 2023 | 161.011 | -60.091 | 0.399 | -6.668 | 1.92 | -28.406 |
| Loktin & Popova | 2017 | 160.995 | -60.087 | â | -6.55 | 2.03 | -13.5 |
| Dias et al. | 2014 | 161.0 | -60.087 | â | -6.31 | 0.12 | â |
| Gozha et al. | 2012 | 161.0 | -60.087 | â | â | â | â |
| Piskunov et al. | 2008 | 160.939 | -60.085 | â | â | â | â |
| Kharchenko et al. | 2007 | 160.99 | -60.09 | â | 0.35 | â | -13.46 |
| van den Bergh | 2006 | 160.95 | -60.083 | â | â | â | â |
| Kharchenko et al. | 2005 | 160.95 | -60.09 | â | -6.66 | 1.93 | -13.46 |
| Kharchenko et al. | 2003 | 160.99 | -60.09 | â | -6.3 | 2.67 | â |
| Chen et al. | 2003 | 160.749 | -59.966 | â | -6.55 | 2.03 | -12.0 |
| Dias et al. | 2002 | 161.0 | -60.087 | â | -6.55 | 2.03 | -10.71 |
| Dambis | 1999 | 161.0 | -60.087 | 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 | 2.2 | 0.96 | 1.06 | 6 | -0.140 | 2975 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 327(1) | â | â |
| Cavallo et al. | 2024 | 1.91 | 0.58 | â | 59 | -0.140 | â | â | â |
| Hunt & Reffert | 2023 | 2.32 | 0.96 | 1.06 | 5 | â | â | â | â |
| Loktin & Popova | 2017 | 1.91 | 1.05 | â | 7 | â | â | â | â |
| Gozha et al. | 2012 | 2.20 | â | â | 7 | â | 5623 | â | â |
| Piskunov et al. | 2008 | 1.91 | 0.81 | â | 5 | â | â | â | â |
| van den Bergh | 2006 | 2.20 | 1.05 | â | 7 | â | â | â | â |
| Kharchenko et al. | 2005 | 1.91 | 0.81 | â | 5 | â | â | â | â |
| Kharchenko et al. | 2003 | 2.22 | 0.93 | â | â | â | â | â | â |
| Chen et al. | 2003 | 2.20 | â | â | 0 | â | â | â | â |
| Dias et al. | 2002 | 2.20 | 1.06 | â | 7 | â | â | â | â |
| Dambis | 1999 | 2.29 | 1.04 | â | 3 | 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)
Silver sample.