MWSC 5634
0.16
UTI
0.0
CN
0.03
Cdens
0.25
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members)
6.4 [arcmin]
- CN 0.0 Sparse
- Cdens 0.03 Very loose
- CC3 0.25 Low quality
- Clit 0.25 Poorly studied
- Cdup 1.0 Unique
Overview
MWSC 5634 is a sparse, very 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 an old cluster (see Parameters). It is poorly studied in the literature.
(*): The parallax distance estimate (~6.24 kpc) differs significantly from the median photometric distance (~1.99 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.
Relatively close
Moderate extinction
Old
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 68.823 | 18.544 | 0.16 | 0.258 | -0.883 | -5.555 |
| Just et al. | 2023 | 68.824 | 18.54 | â | â | â | â |
| Bica et al. | 2019 | 68.818 | 18.539 | â | â | â | â |
| Kharchenko et al. | 2016 | 68.824 | 18.54 | â | â | â | â |
| Schmeja et al. | 2014 | 68.832 | 18.54 | â | 2.81 | -2.88 | 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 | 1778 | â | 316 | â | â |
| Kharchenko et al. | 2016 | 1.99 | 1.48 | â | 1778 | â | â | â | â |
| Schmeja et al. | 2014 | 1.99 | 1.48 | â | 1778 | â | â | â | â |
