CWNU 2619
0.61
UTI
0.54
CN
1.0
Cdens
1.0
CC3
0.31
Clit
0.96
Cdup
Radius (P>50% members)
1.8 [arcmin]
- CN 0.54 Moderately populated
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.31 Poorly studied
- Cdup 0.96 Unique
Overview
CWNU 2619 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the age and metallicity parameters (see Parameters). It was recently reported in the literature.
Note: This is a unique object, which shares a very small percentage of members with at least one previously reported entry. See table with shared members information.
Relatively close
Moderate 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 | 314.902 | 44.964 | 0.321 | -3.571 | -4.559 | -27.32 |
| Zhang et al. | 2024 | 314.901 | 44.97 | â | â | â | â |
| Hunt & Reffert | 2024 | 314.901 | 44.97 | 0.317 | -3.57 | -4.551 | -27.336 |
| Cavallo et al. | 2024 | 314.891 | 44.955 | 0.316 | â | â | â |
| Hunt & Reffert | 2023 | 314.901 | 44.97 | 0.317 | -3.57 | -4.551 | -27.336 |
| He et al. | 2023 | 314.903 | 44.967 | 0.326 | -3.57 | -4.558 | 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 |
|---|---|---|---|---|---|---|---|---|---|
| Zhang et al. | 2024 | â | â | â | â | -0.221* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 383* | â | â |
| Cavallo et al. | 2024 | 2.95 | 1.92 | â | 380 | 0.130 | â | â | â |
| Hunt & Reffert | 2023 | 2.90 | 1.96 | 1.56 | 97 | â | â | â | â |
| He et al. | 2023 | 3.24 | 2.45 | â | 16 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Gold sample.