Turner 11
(MWSC 3403)
0.14
UTI
0.0
CN
0.01
Cdens
0.25
CC3
0.23
Clit
1.0
Cdup
Nm (P>50%)
14
Core radius and density
6.8 [pc], 0.04 [pc-2]
- CN 0.0 Sparse
- Cdens 0.01 Very loose
- CC3 0.25 Low quality
- Clit 0.23 Rarely studied
- Cdup 1.0 Unique
Overview
Turner 11 is a sparse, very loose object of low C3 quality. Its parallax locates it at a large* distance, below the mid-plane, affected by moderate extinction. It is catalogued as an intermediate-age cluster (see Parameters). It is rarely studied in the literature.
(*): The parallax distance estimate (~5.32 kpc) differs significantly from the median photometric distance (~2.20 kpc).
â ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 310.877 | 35.619 | 0.188 | -3.108 | -4.192 | -28.84 |
| Just et al. | 2023 | 310.795 | 35.582 | â | â | â | â |
| Bica et al. | 2019 | 310.848 | 35.589 | â | â | â | â |
| Loktin & Popova | 2017 | 310.845 | 35.588 | â | -0.568 | -1.175 | 10.5 |
| Sampedro et al. | 2017 | 310.85 | 35.588 | â | -2.98 | -4.71 | â |
| Kharchenko et al. | 2016 | 310.795 | 35.582 | â | â | â | â |
| Tadross | 2014 | 310.85 | 35.588 | â | â | â | â |
| Dias et al. | 2014 | 310.85 | 35.588 | â | -3.58 | -5.41 | â |
| Kharchenko et al. | 2013 | 310.8 | 35.585 | â | -2.14 | -3.44 | 10.5 |
| Dias et al. | 2002 | 310.85 | 35.588 | â | -3.58 | -5.41 | 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 | 2.82 | â | 832 | â | 199 | â | â |
| Just et al. | 2023 | â | â | â | 832 | â | 199 | â | â |
| Loktin & Popova | 2017 | 2.47 | 1.43 | â | 1698 | â | â | â | â |
| Kharchenko et al. | 2016 | 2.20 | 2.82 | â | 832 | â | â | â | â |
| Tadross | 2014 | 1.91 | 3.56 | â | 400 | â | â | â | â |
| Kharchenko et al. | 2013 | 2.20 | 2.82 | â | 832 | â | â | â | â |
| Dias et al. | 2002 | 1.91 | 3.56 | â | 398 | â | â | â | â |
MOCA
