DC 5
(Kronberger 38; MWSC 1838; DSH J1039.9-5911; FSR 1549)
0.89
UTI
0.82
CN
1.0
Cdens
1.0
CC3
0.81
Clit
1.0
Cdup
Stellar density (N50/rad)
36.7 [N/pc2]
- CN 0.82 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.81 Well-studied
- Cdup 1.0 Unique
Overview
DC 5 is a rich, very dense object of very high C3 quality. Its parallax locates it at a large distance, near the mid-plane, affected by moderate extinction. It is catalogued as a massive, metal-rich, very young cluster, but with a large variance across recent sources for the age parameter (see Parameters). It is well-studied in the literature.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 159.996 | -59.195 | 0.19 | -5.399 | 2.391 | 4.454 |
| Hunt & Reffert | 2024 | 159.996 | -59.195 | 0.186 | -5.404 | 2.382 | 39.119 |
| Celli et al. | 2024 | 159.996 | -59.192 | â | â | â | â |
| Cavallo et al. | 2024 | 160.006 | -59.192 | 0.186 | â | â | â |
| Hunt & Reffert | 2023 | 159.996 | -59.195 | 0.186 | -5.404 | 2.382 | 39.119 |
| Just et al. | 2023 | 159.99 | -59.187 | â | â | â | â |
| Cantat-Gaudin et al. | 2020 | 159.996 | -59.192 | 0.198 | -5.356 | 2.396 | â |
| Cantat-Gaudin & Anders | 2020 | 159.996 | -59.192 | 0.198 | -5.356 | 2.396 | â |
| Soubiran et al. | 2018 | 159.996 | -59.192 | â | â | â | -4.23 |
| Bica et al. | 2019 | 159.989 | -59.187 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 159.996 | -59.192 | 0.198 | -5.356 | 2.396 | â |
| Kharchenko et al. | 2016 | 159.99 | -59.187 | â | â | â | â |
| Dias et al. | 2014 | 159.996 | -59.189 | â | -5.75 | -2.24 | â |
| Kharchenko et al. | 2013 | 159.997 | -59.19 | â | -7.96 | -0.31 | â |
| Kronberger et al. | 2006 | 159.988 | -59.186 | â | â | â | â |
| Dias et al. | 2002 | 159.996 | -59.189 | â | -7.96 | -0.31 | 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 | 4.42 | 2.58 | 2.54 | 1 | 0.780 | 1885 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 3758(1) | â | â |
| Celli et al. | 2024 | â | â | â | 1 | â | 1885 | â | â |
| Cavallo et al. | 2024 | 3.36 | 3.44 | â | 166 | 0.780 | â | â | â |
| Hunt & Reffert | 2023 | 4.86 | 4.19 | 2.54 | 18 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 1 | â | 1660 | â | â |
| Cantat-Gaudin & Anders | 2020 | 4.41 | â | â | â | â | â | â | â |
| Soubiran et al. | 2018 | 4.41 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 4.41 | â | â | â | â | â | â | â |
| Kharchenko et al. | 2016 | 4.43 | 2.58 | â | 1 | â | â | â | â |
| Kharchenko et al. | 2013 | 4.43 | 2.58 | â | 1 | â | â | â | â |
| Dias et al. | 2002 | 4.43 | 2.58 | â | 1 | 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)
Silver sample.