CWNU 119

Click to load Aladin Lite
0.18 UTI
0.0
CN
0.29
Cdens
0.12
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 18.1 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.29 Loose
  • CC3 0.12 Very low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
CWNU 119 is a sparse, loose object of very low C3 quality. Its parallax locates it at a close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a low-mass, near-solar metallicity, young cluster (see Parameters). It is poorly studied in the literature.

âš 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.

Close Moderate extinction Low mass 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 – 47.433 57.926 1.36 0.915 -5.061 -6.872
Hunt & Reffert 2024 47.45 57.934 1.354 0.886 -5.034 -4.376
Cavallo et al. 2024 47.154 57.952 1.355 – – –
Hunt & Reffert 2023 47.45 57.934 1.354 0.886 -5.034 -4.376
He et al. 2022 47.456 57.938 1.36 0.91 -5.06 –

💡 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 – – – – – 43* – –
Cavallo et al. 2024 0.82 1.93 – 32 0.560 – – –
Hunt & Reffert 2023 0.70 1.95 0.98 57 – – – –
He et al. 2022 0.71 1.98 – 158 0.169 – – –

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

Visualization

â„šī¸