CWNU 324
0.05
UTI
0.44
CN
1.0
Cdens
0.62
CC3
0.25
Clit
0.09
Cdup
Radius (P>50% members)
4.0 [arcmin]
- CN 0.44 Poorly populated
- Cdens 1.0 Very dense
- CC3 0.62 Intermediate quality
- Clit 0.25 Poorly studied
- Cdup 0.09 Very likely duplicate
Overview
CWNU 324 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It is poorly studied in the literature.
â ī¸ Warning: This is very likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.
Relatively close
Moderate extinction
Near-solar metallicity
Very young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 113.006 | -16.942 | 0.525 | -2.207 | 2.558 | â |
| Hunt & Reffert | 2024 | 113.012 | -16.932 | 0.511 | -2.232 | 2.558 | 47.015 |
| Cavallo et al. | 2024 | 113.016 | -16.955 | 0.516 | â | â | â |
| Hunt & Reffert | 2023 | 113.012 | -16.932 | 0.511 | -2.232 | 2.558 | 47.015 |
| He et al. | 2022 | 113.007 | -16.945 | 0.52 | -2.23 | 2.56 | 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 |
|---|---|---|---|---|---|---|---|---|---|
| Hunt & Reffert | 2024 | â | â | â | â | â | 446* | â | â |
| Cavallo et al. | 2024 | 2.08 | 0.93 | â | 25 | 0.280 | â | â | â |
| Hunt & Reffert | 2023 | 1.75 | 1.23 | 2.44 | 18 | â | â | â | â |
| He et al. | 2022 | 2.45 | 1.92 | â | 6 | 0.274 | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.
Cavallo et al. (2024)
Bronze sample.