CWNU 2627
0.37
UTI
0.36
CN
0.25
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members)
9.9 [arcmin]
- CN 0.36 Poorly populated
- Cdens 0.25 Loose
- CC3 0.75 High quality
- Clit 0.25 Poorly studied
- Cdup 1.0 Unique
Overview
CWNU 2627 is a poorly populated, loose object of high C3 quality. Its parallax locates it at a relatively close distance, near 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.
Relatively 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 | 105.167 | -2.874 | 0.532 | -1.535 | 0.952 | 43.038 |
| Hunt & Reffert | 2024 | 105.16 | -2.881 | 0.527 | -1.554 | 0.967 | 43.042 |
| Cavallo et al. | 2024 | 105.158 | -2.895 | 0.528 | â | â | â |
| Hunt & Reffert | 2023 | 105.16 | -2.881 | 0.527 | -1.554 | 0.967 | 43.042 |
| He et al. | 2023 | 105.074 | -2.874 | 0.539 | -1.533 | 0.935 | 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 | 102* | â | â |
| Cavallo et al. | 2024 | 1.62 | 0.47 | â | 87 | -0.260 | â | â | â |
| Hunt & Reffert | 2023 | 1.76 | 0.16 | 0.44 | 126 | â | â | â | â |
| He et al. | 2023 | 1.95 | 0.50 | â | 45 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.
Cavallo et al. (2024)
Gold sample.