Basel 7
(MWSC 932)
0.17
UTI
0.0
CN
0.02
Cdens
0.12
CC3
0.35
Clit
1.0
Cdup
Nm (P>50%)
18
Core radius and density
3.3 [pc], 0.1 [pc-2]
- CN 0.0 Sparse
- Cdens 0.02 Very loose
- CC3 0.12 Very low quality
- Clit 0.35 Poorly studied
- Cdup 1.0 Unique
Overview
Basel 7 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a large* distance, above the mid-plane, affected by moderate extinction. It is catalogued as a low-mass, intermediate-age cluster (see Parameters). It is poorly studied in the literature.
(*): The parallax distance estimate (~5.26 kpc) differs significantly from the median photometric distance (~1.62 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 | 99.119 | 8.352 | 0.19 | 0.119 | -0.213 | 35.142 |
| Just et al. | 2023 | 99.068 | 8.331 | â | â | â | â |
| Dib et al. | 2018 | 99.075 | 8.33 | â | â | â | â |
| Loktin & Popova | 2017 | 99.15 | 8.35 | â | -0.47 | -0.428 | â |
| Sampedro et al. | 2017 | 99.15 | 8.35 | â | 0.23 | 0.59 | â |
| Joshi et al. | 2016 | 99.075 | 8.33 | â | â | â | â |
| Kharchenko et al. | 2016 | 99.068 | 8.331 | â | â | â | â |
| Dias et al. | 2014 | 99.15 | 8.35 | â | 0.31 | 0.47 | â |
| Kharchenko et al. | 2013 | 99.075 | 8.33 | â | -2.59 | -1.75 | â |
| Bukowiecki et al. | 2011 | 99.333 | 8.156 | â | â | â | â |
| van den Bergh | 2006 | 99.15 | 8.35 | â | â | â | â |
| Dias et al. | 2002 | 99.15 | 8.35 | â | 0.31 | 0.47 | â |
| Lynga | 1987 | 99.156 | 8.36 | â | â | â | 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 | 1.62 | 1.26 | â | 127 | â | 46 | â | â |
| Just et al. | 2023 | â | â | â | 127 | â | 39 | â | â |
| Dib et al. | 2018 | 1.56 | â | â | 127 | â | â | â | â |
| Loktin & Popova | 2017 | 1.77 | 1.24 | â | 131 | â | â | â | â |
| Joshi et al. | 2016 | 1.56 | 1.31 | â | 127 | â | â | â | â |
| Kharchenko et al. | 2016 | 1.56 | 1.31 | â | 127 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.56 | 1.31 | â | 127 | â | â | â | â |
| Bukowiecki et al. | 2012 | â | â | â | â | â | 52 | â | â |
| Bukowiecki et al. | 2011 | 1.95(1) | 1.14 | â | 89 | â | â | â | â |
| van den Bergh | 2006 | 1.68 | 1.26 | â | 107 | â | â | â | â |
| Dias et al. | 2002 | 1.68 | 1.25 | â | 108 | â | â | â | â |
| Lynga | 1987 | â | â | â | 631 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA
