CWNU 395
0.44
UTI
0.34
CN
0.61
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad)
3.1 [N/pc2]
- CN 0.34 Poorly populated
- Cdens 0.61 Moderately dense
- CC3 0.75 High quality
- Clit 0.25 Poorly studied
- Cdup 1.0 Unique
đĨ Members
đ Colab
đŦ Bayestar19
MOCA
đ CDS
đ Simbad
đ CDS (Îą, δ)
đ Simbad (Îą, δ)
MOCA
đ CDS
đ Simbad
đ CDS (Îą, δ)
đ Simbad (Îą, δ)
Overview
CWNU 395 is a poorly populated, moderately dense object of high 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, intermediate-age cluster, but with a large variance across recent sources for the age parameter (see Parameters). It is poorly studied in the literature.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 229.232 | -53.687 | 0.549 | -0.741 | -1.426 | â |
| Hunt & Reffert | 2024 | 229.237 | -53.677 | 0.541 | -0.755 | -1.415 | â |
| Cavallo et al. | 2024 | 229.243 | -53.679 | 0.543 | â | â | â |
| Hunt & Reffert | 2023 | 229.237 | -53.677 | 0.541 | -0.755 | -1.415 | â |
| He et al. | 2022 | 229.234 | -53.682 | 0.54 | -0.76 | -1.4 | 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] | Bfrac | BSS |
|---|---|---|---|---|---|---|---|---|---|
| UCC | 99999â | 1.77 | 1.15 | 0.44 | 125 | 0.439 | 227 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 227(1) | â | â |
| Cavallo et al. | 2024 | 1.77 | 1.48 | â | 81 | 0.340 | â | â | â |
| Hunt & Reffert | 2023 | 1.72 | 1.15 | 0.44 | 125 | â | â | â | â |
| He et al. | 2022 | 1.95 | 1.14 | â | 316 | 0.537 | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
Cavallo et al. (2024)
Gold sample.