Dias 7
(MWSC 3188)
0.14
UTI
0.0
CN
0.01
Cdens
0.12
CC3
0.29
Clit
1.0
Cdup
Nm (P>50%)
15
Core radius and density
6.6 [pc], 0.07 [pc-2]
- CN 0.0 Sparse
- Cdens 0.01 Very loose
- CC3 0.12 Very low quality
- Clit 0.29 Poorly studied
- Cdup 1.0 Unique
Overview
Dias 7 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a large* distance, below the mid-plane, affected by moderate extinction. It is catalogued as an old cluster (see Parameters). It is poorly studied in the literature.
(*): The parallax distance estimate (~5.25 kpc) differs significantly from the median photometric distance (~2.65 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 | 297.358 | 21.177 | 0.191 | -3.527 | -5.038 | -48.721 |
| Just et al. | 2023 | 297.361 | 21.165 | â | â | â | â |
| Bica et al. | 2019 | 297.327 | 21.142 | â | â | â | â |
| Dias et al. | 2018 | â | â | â | -4.48 | -5.72 | â |
| Loktin & Popova | 2017 | 297.345 | 21.17 | â | -4.968 | -14.711 | â |
| Sampedro et al. | 2017 | 297.337 | 21.17 | â | 0.57 | -6.19 | â |
| Kharchenko et al. | 2016 | 297.361 | 21.165 | â | â | â | â |
| Tadross | 2014 | 297.342 | 21.163 | â | â | â | â |
| Dias et al. | 2014 | 297.337 | 21.17 | â | 0.48 | -6.19 | â |
| Kharchenko et al. | 2013 | 297.367 | 21.167 | â | -1.17 | -14.18 | â |
| Bukowiecki et al. | 2011 | 297.346 | 21.172 | â | â | â | â |
| Dias et al. | 2002 | 297.337 | 21.17 | â | 0.48 | -6.19 | 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 | 2.65 | 1.435 | â | 2089 | â | 275 | â | â |
| Just et al. | 2023 | â | â | â | 2089 | â | 275 | â | â |
| Loktin & Popova | 2017 | 2.30 | 0.84 | â | 2630 | â | â | â | â |
| Kharchenko et al. | 2016 | 2.80 | 1.64 | â | 2089 | â | â | â | â |
| Tadross | 2014 | 2.54 | 1.32 | â | 2000 | â | â | â | â |
| Kharchenko et al. | 2013 | 2.80 | 1.64 | â | 2089 | â | â | â | â |
| Bukowiecki et al. | 2011 | 2.76(1) | 1.55 | â | 2818 | â | â | â | â |
| Dias et al. | 2002 | 2.54 | 1.32 | â | 1995 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA

Bica et al. (2019)
Web updates in DAML02, some were later removed (2003 to 2010).