Collinder 471
(MWSC 3587)
0.63
UTI
0.27
CN
1.0
Cdens
1.0
CC3
0.45
Clit
1.0
Cdup
Stellar density (N50/rad)
14.1 [N/pc2]
- CN 0.27 Poorly populated
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.45 Poorly studied
- Cdup 1.0 Unique
Overview
Collinder 471 is a poorly populated, very dense object of very high C3 quality. Its parallax locates it at a very close* distance, above the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, very young cluster, but with a large variance across recent sources for the age parameter (see Parameters). It is poorly studied in the literature.
(*): The parallax distance estimate (~0.34 kpc) differs significantly from the median photometric distance (~2.00 kpc).
Note: This object shares a large percentage of members with 2 later reported entries. 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 | 332.562 | 73.025 | 2.923 | 5.334 | 1.565 | -17.775 |
| Cavallo et al. | 2024 | 333.393 | 73.346 | 2.928 | â | â | â |
| Hunt & Reffert | 2023 | 332.563 | 73.032 | 2.93 | 5.321 | 1.632 | -22.556 |
| Just et al. | 2023 | 331.682 | 71.972 | â | â | â | â |
| Kharchenko et al. | 2016 | 331.682 | 71.972 | â | â | â | â |
| Dias et al. | 2014 | 331.775 | 72.0 | â | -2.22 | -3.32 | -10.94 |
| Kharchenko et al. | 2013 | 331.687 | 71.975 | â | 4.09 | -2.09 | â |
| Kharchenko et al. | 2012 | 331.702 | 71.978 | â | 3.09 | -2.81 | â |
| Dias et al. | 2002 | 331.775 | 72.0 | â | -2.22 | -3.32 | -10.94 |
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 | 2.0 | 3.1 | 1.39 | 8 | 0.140 | 427 | â | â |
| Cavallo et al. | 2024 | 0.34 | 1.64 | â | 5 | 0.140 | â | â | â |
| Hunt & Reffert | 2023 | 0.33 | 0.75 | 1.39 | 5 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 631 | â | 427 | â | â |
| Kharchenko et al. | 2016 | 2.21 | 3.16 | â | 631 | â | â | â | â |
| Kharchenko et al. | 2013 | 2.21 | 3.16 | â | 631 | â | â | â | â |
| Kharchenko et al. | 2012 | 2.00 | 3.10 | â | 8 | â | â | â | â |
| Dias et al. | 2002 | 2.00 | 3.10 | â | 8 | â | â | â | â |
MOCA


Cantat-Gaudin et al. (2020)
Catalogue parameters are highly discrepant. No clear radius or kinematic signature identified. More details in Appendix A of the article.
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as a moving group.