NGC 7093
(MWSC 3528)
0.25
UTI
0.0
CN
0.02
Cdens
0.25
CC3
0.5
Clit
1.0
Cdup
Radius (P>50% members)
5.9 [arcmin]
- CN 0.0 Sparse
- Cdens 0.02 Very loose
- CC3 0.25 Low quality
- Clit 0.5 Moderately studied
- Cdup 1.0 Unique
Overview
NGC 7093 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 a near-solar metallicity, intermediate-age cluster (see Parameters). It is moderately studied in the literature.
(*): The parallax distance estimate (~6.30 kpc) differs significantly from the median photometric distance (~2.50 kpc).
Relatively close
Moderate extinction
Near-solar metallicity
Intermediate age
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 323.688 | 45.978 | 0.159 | -2.868 | -2.26 | â |
| Just et al. | 2023 | 323.604 | 45.911 | â | â | â | â |
| Bica et al. | 2019 | 323.671 | 46.016 | â | â | â | â |
| Loktin & Popova | 2017 | 323.61 | 45.965 | â | -1.098 | -1.546 | â |
| Kharchenko et al. | 2016 | 323.604 | 45.911 | â | â | â | â |
| Dias et al. | 2014 | 323.587 | 45.965 | â | -1.96 | -3.57 | â |
| Kharchenko et al. | 2013 | 323.61 | 45.915 | â | -2.65 | -4.06 | â |
| Kharchenko et al. | 2012 | 323.61 | 45.915 | â | -2.65 | -4.06 | â |
| Dias et al. | 2002 | 323.587 | 45.965 | â | -1.96 | -3.57 | 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] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Just et al. | 2023 | â | â | â | 316 | â | 371 | â | â |
| Loktin & Popova | 2017 | 2.54 | 0.60 | â | 1514 | â | â | â | â |
| Kharchenko et al. | 2016 | 2.50 | 2.73 | â | 316 | â | â | â | â |
| Kharchenko et al. | 2013 | 2.50 | 2.73 | â | 316 | â | â | â | â |
| Kharchenko et al. | 2012 | 2.50 | 2.73 | â | 316 | â | â | â | â |
| Dias et al. | 2002 | 1.78 | 1.89 | â | 891 | -0.150 | â | â | â |
