DC 8
(MWSC 758; Teutsch J0609.3+3113)
0.68
UTI
0.52
CN
1.0
Cdens
0.5
CC3
0.69
Clit
1.0
Cdup
Stellar density (N50/rad)
22.1 [N/pc2]
- CN 0.52 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.5 Intermediate quality
- Clit 0.69 Moderately studied
- Cdup 1.0 Unique
Overview
DC 8 is a moderately populated, very dense object of intermediate C3 quality. Its parallax locates it at a large* distance, well above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the mass parameter (see Parameters). It is moderately studied in the literature.
(*): The parallax distance estimate (~5.32 kpc) differs significantly from the median photometric distance (~3.97 kpc).
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 92.338 | 31.226 | 0.188 | 0.7 | -1.212 | 13.855 |
| Hunt & Reffert | 2024 | 92.339 | 31.226 | 0.173 | 0.695 | -1.238 | 13.857 |
| Cavallo et al. | 2024 | 92.34 | 31.226 | 0.176 | â | â | â |
| Hunt & Reffert | 2023 | 92.339 | 31.226 | 0.173 | 0.695 | -1.238 | 13.857 |
| Just et al. | 2023 | 92.32 | 31.224 | â | â | â | â |
| Cantat-Gaudin et al. | 2020 | 92.335 | 31.228 | 0.223 | 0.775 | -1.309 | â |
| Cantat-Gaudin & Anders | 2020 | 92.335 | 31.228 | 0.223 | 0.775 | -1.309 | â |
| Bica et al. | 2019 | 92.338 | 31.225 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 92.335 | 31.228 | 0.223 | 0.775 | -1.309 | â |
| Kharchenko et al. | 2016 | 92.32 | 31.224 | â | â | â | â |
| Kharchenko et al. | 2013 | 92.329 | 31.223 | â | 0.07 | -4.45 | â |
| Glushkova et al. | 2010 | 92.339 | 31.232 | â | â | â | â |
| Dias et al. | 2002 | 92.338 | 31.232 | â | 0.07 | -4.45 | 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 | 3.97 | 2.84 | 2.26 | 453 | -0.090 | 258 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 473(1) | â | â |
| Cavallo et al. | 2024 | 4.92 | 3.44 | â | 427 | -0.090 | â | â | â |
| Hunt & Reffert | 2023 | 4.04 | 2.84 | 2.26 | 479 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 403 | â | 42 | â | â |
| Cantat-Gaudin et al. | 2020 | 4.59 | 2.51 | â | 851 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 3.97 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 3.97 | â | â | â | â | â | â | â |
| Kharchenko et al. | 2016 | 2.71 | 3.23 | â | 403 | â | â | â | â |
| Kharchenko et al. | 2013 | 2.71 | 3.23 | â | 403 | â | â | â | â |
| Glushkova et al. | 2010 | 2.10 | 2.23 | â | 1000 | â | â | â | â |
| Dias et al. | 2002 | 2.10 | 2.23 | â | 1000 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Cavallo et al. (2024)
Gold sample.