MWSC 5044
0.35
UTI
0.25
CN
1.0
Cdens
0.5
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members)
10.1 [arcmin]
- CN 0.25 Poorly populated
- Cdens 1.0 Very dense
- CC3 0.5 Intermediate quality
- Clit 0.0 Rarely studied
- Cdup 1.0 Unique
Overview
MWSC 5044 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a very close* distance, above the mid-plane, affected by low extinction. It is catalogued as an old cluster (see Parameters). It is rarely studied in the literature.
(*): The parallax distance estimate (~0.41 kpc) differs significantly from the median photometric distance (~2.73 kpc).
Relatively close
Low extinction
Old
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 141.179 | 29.99 | 2.467 | -15.644 | -14.256 | 9.483 |
| Just et al. | 2023 | 141.278 | 29.928 | â | â | â | â |
| Bica et al. | 2019 | 141.273 | 29.927 | â | â | â | â |
| Schmeja et al. | 2014 | 141.285 | 29.925 | â | -5.72 | -5.25 | 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 | 3715 | â | 299 | â | â |
| Schmeja et al. | 2014 | 2.73 | 0.19 | â | 3715 | â | â | â | â |
