Turner 1
(MWSC 3184)
0.21
UTI
0.0
CN
0.05
Cdens
0.12
CC3
0.44
Clit
1.0
Cdup
Radius (P>50% members)
6.3 [arcmin]
- CN 0.0 Sparse
- Cdens 0.05 Very loose
- CC3 0.12 Very low quality
- Clit 0.44 Poorly studied
- Cdup 1.0 Unique
Overview
Turner 1 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a moderate* distance, above the mid-plane, affected by moderate extinction. It is catalogued as an intermediate-age cluster (see Parameters). It is poorly studied in the literature.
(*): The parallax distance estimate (~3.92 kpc) differs significantly from the median photometric distance (~2.79 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.
Relatively close
Moderate extinction
Intermediate age
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 297.118 | 27.281 | 0.255 | -3.795 | -6.529 | -67.629 |
| Just et al. | 2023 | 297.107 | 27.293 | â | â | â | â |
| Loktin & Popova | 2017 | 297.12 | 27.298 | â | -3.802 | -2.805 | 0.5 |
| Kharchenko et al. | 2016 | 297.107 | 27.293 | â | â | â | â |
| Dias et al. | 2014 | 297.104 | 27.293 | â | -3.48 | -3.81 | 0.5 |
| Kharchenko et al. | 2013 | 297.112 | 27.295 | â | -4.39 | -3.22 | â |
| van den Bergh | 2006 | 297.267 | 27.298 | â | â | â | â |
| Dias et al. | 2002 | 297.104 | 27.293 | â | -3.48 | -3.81 | 0.5 |
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] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Just et al. | 2023 | â | â | â | 550 | â | 350 | â | â |
| Loktin & Popova | 2017 | 3.98 | 1.58 | â | 1023 | â | â | â | â |
| Kharchenko et al. | 2016 | 2.79 | 1.68 | â | 550 | â | â | â | â |
| Kharchenko et al. | 2013 | 2.79 | 1.68 | â | 550 | â | â | â | â |
| van den Bergh | 2006 | 1.68 | 1.49 | â | 29 | â | â | â | â |
| Dias et al. | 2002 | 1.68 | 1.48 | â | 29 | â | â | â | â |
