CWNU 1470
0.38
UTI
0.3
CN
0.35
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad)
1.7 [N/pc2]
- CN 0.3 Poorly populated
- Cdens 0.35 Loose
- 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 1470 is a poorly populated, loose object of high C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 179.737 | -55.608 | 0.506 | -6.93 | 0.696 | -36.401 |
| Hunt & Reffert | 2024 | 179.761 | -55.617 | 0.476 | -6.905 | 0.767 | -55.704 |
| Cavallo et al. | 2024 | 179.743 | -55.618 | 0.494 | â | â | â |
| Hunt & Reffert | 2023 | 179.761 | -55.617 | 0.476 | -6.905 | 0.767 | -55.704 |
| He et al. | 2023 | 179.693 | -55.602 | 0.512 | -6.931 | 0.715 | 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 | 1.86 | 0.6 | 0.53 | 94 | -0.290 | 141 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 141(1) | â | â |
| Cavallo et al. | 2024 | 1.71 | 0.61 | â | 141 | -0.290 | â | â | â |
| Hunt & Reffert | 2023 | 1.87 | 0.34 | 0.53 | 94 | â | â | â | â |
| He et al. | 2023 | 1.86 | 0.60 | â | 40 | â | 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.