Turner 6
(MWSC 1876)
0.76
UTI
0.68
CN
1.0
Cdens
1.0
CC3
0.55
Clit
1.0
Cdup
Stellar density (N50/rad)
11.3 [N/pc2]
- CN 0.68 Moderately populated
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.55 Moderately studied
- Cdup 1.0 Unique
Overview
Turner 6 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a large* distance, above the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the age parameter (see Parameters). It is moderately studied in the literature.
(*): The parallax distance estimate (~7.96 kpc) differs significantly from the median photometric distance (~4.38 kpc).
Note: This object shares a large percentage of members with at least one entry reported in the same catalogue. 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 | 164.833 | -59.543 | 0.126 | -6.011 | 2.12 | 51.24 |
| Hunt & Reffert | 2024 | 164.834 | -59.544 | 0.119 | -5.999 | 2.144 | 51.905 |
| Cavallo et al. | 2024 | 164.823 | -59.555 | 0.118 | â | â | â |
| Hunt & Reffert | 2023 | 164.834 | -59.544 | 0.119 | -5.999 | 2.144 | 51.905 |
| Just et al. | 2023 | 164.746 | -59.479 | â | â | â | â |
| Kharchenko et al. | 2016 | 164.746 | -59.479 | â | â | â | â |
| Dias et al. | 2014 | 164.754 | -59.499 | â | 0.58 | 0.34 | â |
| Kharchenko et al. | 2013 | 164.754 | -59.483 | â | -0.88 | -0.4 | â |
| Bukowiecki et al. | 2011 | 164.746 | -59.503 | â | â | â | â |
| Dias et al. | 2002 | 164.754 | -59.499 | â | 0.72 | 1.76 | 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 | 4.375 | 3.55 | 2.33 | 79 | -0.180 | 661 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 1111(1) | â | â |
| Cavallo et al. | 2024 | 5.15 | 2.19 | â | 776 | -0.180 | â | â | â |
| Hunt & Reffert | 2023 | 8.15 | 2.79 | 2.33 | 225 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 4 | â | 661 | â | â |
| Kharchenko et al. | 2016 | 3.60 | 3.55 | â | 4 | â | â | â | â |
| Kharchenko et al. | 2013 | 3.60 | 3.55 | â | 4 | â | â | â | â |
| Bukowiecki et al. | 2012 | â | â | â | â | â | 148 | â | â |
| Bukowiecki et al. | 2011 | 5.55(1) | 5.27 | â | 79 | â | â | â | â |
| Dias et al. | 2002 | 3.25 | 4.09 | â | 79 | 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.