CWNU 2475

Click to load Aladin Lite
0.36 UTI
0.5
CN
0.57
Cdens
0.25
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 4.9 [arcmin]
  • CN 0.5 Moderately populated
  • Cdens 0.57 Moderately dense
  • CC3 0.25 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
CWNU 2475 is a moderately populated, moderately dense object of low C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.
Relatively close High extinction Near-solar metallicity Young

Cavallo et al. (2024)
Silver sample.

Data

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 212.021 -60.486 0.34 -4.256 -2.248 -7.646
Hunt & Reffert 2024 212.036 -60.493 0.337 -4.268 -2.284 -7.604
Cavallo et al. 2024 212.044 -60.48 0.337 – – –
Hunt & Reffert 2023 212.036 -60.493 0.337 -4.268 -2.284 -7.604
He et al. 2023 212.04 -60.489 0.35 -4.271 -2.251 -7.65

💡 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 – – – – – 279* – –
Cavallo et al. 2024 2.26 3.85 – 81 0.040 – – –
Hunt & Reffert 2023 2.95 3.65 1.72 78 – – – –
He et al. 2023 3.09 1.70 – 1 – – – –

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

Visualization

â„šī¸