CWNU 477

Click to load Aladin Lite
0.55 UTI
0.48
CN
1.0
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 4.3 [arcmin]
  • CN 0.48 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
CWNU 477 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, above 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 – 273.018 -15.693 0.655 1.119 -1.45 -18.305
Hunt & Reffert 2024 273.015 -15.694 0.647 1.08 -1.53 -18.301
Cavallo et al. 2024 273.031 -15.701 0.647 – – –
Hunt & Reffert 2023 273.015 -15.694 0.647 1.08 -1.53 -18.301
He et al. 2022 273.017 -15.704 0.66 1.08 -1.46 –

💡 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 – – – – – 161* – –
Cavallo et al. 2024 1.20 1.49 – 490 -0.640 – – –
Hunt & Reffert 2023 1.45 1.40 1.42 147 – – – –
He et al. 2022 1.45 0.06 – 8 0.169 – – –

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

Visualization

â„šī¸