CWNU 2105
0.24
UTI
0.0
CN
0.33
Cdens
0.38
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members)
8.4 [arcmin]
- CN 0.0 Sparse
- Cdens 0.33 Loose
- CC3 0.38 Low quality
- Clit 0.25 Poorly studied
- Cdup 1.0 Unique
Overview
CWNU 2105 is a sparse, loose object of low C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It was recently reported in the literature.
â ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.
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 | 87.345 | 27.028 | 0.654 | 0.116 | -2.411 | 16.022 |
| Hunt & Reffert | 2024 | 87.353 | 27.041 | 0.642 | 0.156 | -2.468 | 15.982 |
| Cavallo et al. | 2024 | 87.386 | 27.024 | 0.641 | â | â | â |
| Hunt & Reffert | 2023 | 87.353 | 27.041 | 0.642 | 0.156 | -2.468 | 15.982 |
| He et al. | 2023 | 87.359 | 27.031 | 0.654 | 0.096 | -2.451 | 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 | 98* | â | â |
| Cavallo et al. | 2024 | 1.81 | 1.46 | â | 10 | -0.110 | â | â | â |
| Hunt & Reffert | 2023 | 1.47 | 1.52 | 1.53 | 15 | â | â | â | â |
| He et al. | 2023 | 1.62 | 1.75 | â | 7 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.
Cavallo et al. (2024)
Silver sample.