CWNU 2573

Click to load Aladin Lite
0.56 UTI
0.28
CN
1.0
Cdens
1.0
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 1.7 [arcmin]
  • CN 0.28 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
CWNU 2573 is a poorly populated, very dense object of very high 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, young cluster (see Parameters). It was recently reported in the literature.
Relatively close Moderate extinction Near-solar metallicity Young

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 – 203.192 -63.853 0.339 -5.759 -2.418 -32.004
Hunt & Reffert 2024 203.185 -63.846 0.335 -5.764 -2.418 -31.923
Cavallo et al. 2024 203.208 -63.855 0.339 – – –
Hunt & Reffert 2023 203.185 -63.846 0.335 -5.764 -2.418 -31.923
He et al. 2023 203.191 -63.842 0.339 -5.756 -2.424 -32.0

💡 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 – – – – – 449* – –
Cavallo et al. 2024 2.33 1.40 – 66 -0.150 – – –
Hunt & Reffert 2023 2.76 1.32 0.81 54 – – – –
He et al. 2023 2.82 1.40 – 8 – – – –

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

Visualization

â„šī¸