CWNU 1857

Click to load Aladin Lite
0.47 UTI
0.32
CN
0.63
Cdens
0.75
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members) 7.3 [arcmin]
  • CN 0.32 Poorly populated
  • Cdens 0.63 Moderately dense
  • CC3 0.75 High quality
  • Clit 0.31 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
CWNU 1857 is a poorly populated, moderately dense 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, but with a large variance across recent sources for the metallicity parameter (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 – 281.934 -6.167 0.667 -1.827 1.701 -0.764
Hu & Soubiran 2025 281.98 -6.137 – – – –
Hunt & Reffert 2024 281.963 -6.076 0.662 -1.806 1.711 -0.685
Cavallo et al. 2024 281.98 -6.137 0.665 – – –
Hunt & Reffert 2023 281.963 -6.076 0.662 -1.806 1.711 -0.685
He et al. 2023 281.927 -6.222 0.667 -1.827 1.689 -0.76

💡 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
Hu & Soubiran 2025 – – – – -0.130* – – –
Hunt & Reffert 2024 – – – – – 310* – –
Cavallo et al. 2024 1.20 2.04 – 955 -0.580 – – –
Hunt & Reffert 2023 1.45 1.49 1.48 640 – – – –
He et al. 2023 1.48 1.40 – 1413 – – – –

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

Visualization

â„šī¸