CWNU 66

Click to load Aladin Lite
0.44 UTI
0.31
CN
1.0
Cdens
0.38
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 3.2 [arcmin]
  • CN 0.31 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 66 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, intermediate-age cluster (see Parameters). It is poorly studied 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 – 33.311 61.472 0.412 -0.067 -0.755 -45.33
Hunt & Reffert 2024 33.355 61.465 0.407 -0.094 -0.78 -45.332
Cavallo et al. 2024 33.339 61.478 0.41 – – –
Hunt & Reffert 2023 33.355 61.465 0.407 -0.094 -0.78 -45.332
He et al. 2022 33.307 61.454 0.41 -0.09 -0.76 -45.3

💡 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 – – – – – 435* – –
Cavallo et al. 2024 1.94 3.00 – 115 -0.390 – – –
Hunt & Reffert 2023 2.28 2.95 1.87 142 – – – –
He et al. 2022 2.75 3.54 – 25 0.169 – – –

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

Visualization

â„šī¸