CWNU 2672
0.61
UTI
0.53
CN
1.0
Cdens
1.0
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members)
2.5 [arcmin]
- CN 0.53 Moderately populated
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.25 Poorly studied
- Cdup 1.0 Unique
Overview
CWNU 2672 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 very high extinction. It is catalogued as a massive, near-solar metallicity, very young cluster, but with a large variance across recent sources for the age parameter (see Parameters). It was recently reported in the literature.
Distant
Very high extinction
Massive
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 | 251.595 | -45.183 | 0.271 | -1.899 | -3.163 | -49.626 |
| Hunt & Reffert | 2024 | 251.57 | -45.207 | 0.28 | -1.912 | -3.166 | -39.008 |
| Cavallo et al. | 2024 | 251.6 | -45.193 | 0.279 | â | â | â |
| Hunt & Reffert | 2023 | 251.57 | -45.207 | 0.28 | -1.912 | -3.166 | -39.008 |
| He et al. | 2023 | 251.597 | -45.179 | 0.279 | -1.898 | -3.143 | -55.23 |
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 | 2483* | â | â |
| Cavallo et al. | 2024 | 5.40 | 5.06 | â | 1 | 0.180 | â | â | â |
| Hunt & Reffert | 2023 | 3.19 | 6.53 | 2.71 | 18 | â | â | â | â |
| He et al. | 2023 | 3.09 | 7.60 | â | 16 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.
Cavallo et al. (2024)
Wood sample.