CWNU 2314

Click to load Aladin Lite
0.35 UTI
0.3
CN
0.22
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 9.8 [arcmin]
  • CN 0.3 Poorly populated
  • Cdens 0.22 Very loose
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
CWNU 2314 is a poorly populated, very loose object of high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.
Relatively close Moderate extinction Near-solar metallicity Intermediate age

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 – 273.382 -21.366 0.54 0.719 -0.183 55.944
Hunt & Reffert 2024 273.397 -21.377 0.536 0.716 -0.169 55.945
Cavallo et al. 2024 273.406 -21.314 0.538 – – –
Hunt & Reffert 2023 273.397 -21.377 0.536 0.716 -0.169 55.945
He et al. 2023 273.377 -21.364 0.542 0.721 -0.183 –

💡 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 – – – – – 232* – –
Cavallo et al. 2024 1.55 2.01 – 209 -0.080 – – –
Hunt & Reffert 2023 1.73 1.96 1.79 103 – – – –
He et al. 2023 1.70 2.45 – 35 – – – –

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

Visualization

â„šī¸