CWNU 410
(OCSN 153)
0.43
UTI
0.53
CN
0.37
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members)
43.8 [arcmin]
- CN 0.53 Moderately populated
- Cdens 0.37 Loose
- CC3 0.75 High quality
- Clit 0.25 Poorly studied
- Cdup 1.0 Unique
Overview
CWNU 410 is a moderately populated, loose object of high C3 quality. Its parallax locates it at a very close distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is poorly studied in the literature.
Very close
Low extinction
Near-solar metallicity
Young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 96.949 | -13.153 | 2.305 | -4.375 | 3.834 | 39.227 |
| Cavallo et al. | 2024 | 96.757 | -13.008 | 2.315 | â | â | â |
| Hunt & Reffert | 2023 | 96.126 | -12.957 | 2.313 | -4.443 | 3.798 | 37.078 |
| Qin et al. | 2023 | 96.99 | -13.49 | 2.31 | -4.39 | 3.78 | 38.33 |
| He et al. | 2022 | 97.171 | -13.582 | 2.22 | -4.36 | 3.88 | 39.5 |
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 |
|---|---|---|---|---|---|---|---|---|---|
| Cavallo et al. | 2024 | 0.44 | 0.42 | â | 68 | 0.500 | â | â | â |
| Hunt & Reffert | 2023 | 0.42 | 0.21 | 0.57 | 76 | â | â | â | â |
| Qin et al. | 2023 | 0.52 | 0.40 | â | 40 | â | â | â | â |
| He et al. | 2022 | 0.46 | 0.36 | â | 50 | 0.457 | â | â | â |
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as a moving group.