CWNU 1866

Click to load Aladin Lite
0.43 UTI
0.25
CN
1.0
Cdens
0.38
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 2.8 [arcmin]
  • CN 0.25 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.38 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
CWNU 1866 is a poorly populated, very dense object of low 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 (see Parameters). It was recently reported in the literature.
Relatively close Moderate extinction Near-solar metallicity Young

Cavallo et al. (2024)
Gold sample.

Data

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 190.303 -62.454 0.425 -4.453 -0.843 -2.404
Hunt & Reffert 2024 190.353 -62.438 0.42 -4.459 -0.825 –
Cavallo et al. 2024 190.314 -62.431 0.423 – – –
Hunt & Reffert 2023 190.353 -62.438 0.42 -4.459 -0.825 –
He et al. 2023 190.264 -62.435 0.437 -4.451 -0.862 –

💡 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 – – – – – 130* – –
Cavallo et al. 2024 2.41 2.74 – 40 0.110 – – –
Hunt & Reffert 2023 2.16 2.38 2.21 71 – – – –
He et al. 2023 2.09 2.55 – 251 – – – –

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Visualization

â„šī¸