DC 4
(MWSC 1010)
0.23
UTI
0.0
CN
0.26
Cdens
0.25
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members)
1.6 [arcmin]
- CN 0.0 Sparse
- Cdens 0.26 Loose
- CC3 0.25 Low quality
- Clit 0.31 Poorly studied
- Cdup 1.0 Unique
Overview
DC 4 is a sparse, loose object of low C3 quality. Its parallax locates it at a large* distance, well below 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 (~9.02 kpc) differs significantly from the median photometric distance (~2.30 kpc).
Note: This object shares a significant percentage of members with a later reported entry. See table with shared members information.
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.
Relatively close
Moderate extinction
Low mass
Intermediate age
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 103.514 | -13.566 | 0.111 | -0.358 | 0.743 | 96.702 |
| Just et al. | 2023 | 103.517 | -13.554 | â | â | â | â |
| Bica et al. | 2019 | 103.516 | -13.567 | â | â | â | â |
| Kharchenko et al. | 2016 | 103.517 | -13.554 | â | â | â | â |
| Kharchenko et al. | 2013 | 103.522 | -13.555 | â | 4.88 | -3.34 | â |
| Dias et al. | 2002 | 103.513 | -13.568 | â | 4.88 | -3.34 | 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 | 501 | â | 41 | â | â |
| Kharchenko et al. | 2016 | 2.30 | 1.81 | â | 501 | â | â | â | â |
| Kharchenko et al. | 2013 | 2.30 | 1.81 | â | 501 | â | â | â | â |
| Dias et al. | 2002 | 2.30 | 1.81 | â | 501 | â | â | â | â |
