CWNU 2479

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0.31 UTI
0.41
CN
1.0
Cdens
0.25
CC3
0.25
Clit
0.71
Cdup
Radius (P>50% members) 3.8 [arcmin]
  • CN 0.41 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.25 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 0.71 Likely unique

Overview

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CWNU 2479 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 high extinction. It is catalogued as a metal-rich, intermediate-age cluster, but with a large variance across recent sources for the age parameter (see Parameters). It was recently reported in the literature.

Note: This is likely a unique object, which shares a moderate percentage of members with at least one previously reported entry. See table with shared members information.

Relatively close High extinction Metal-rich Intermediate age

Cavallo et al. (2024)
Gold sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 243.142 -50.913 0.396 -2.358 -3.05 -52.282
Hunt & Reffert 2024 243.125 -50.925 0.396 -2.376 -3.083 –
Cavallo et al. 2024 243.149 -50.919 0.392 – – –
Hunt & Reffert 2023 243.125 -50.925 0.396 -2.376 -3.083 –
He et al. 2023 243.141 -50.923 0.401 -2.353 -3.046 -52.28

💡 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 – – – – – 411* – –
Cavallo et al. 2024 2.63 2.53 – 141 0.990 – – –
Hunt & Reffert 2023 2.43 3.31 1.75 26 – – – –
He et al. 2023 2.57 3.50 – 141 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Ryu 292 29.3 243.14 -50.95 0.41 -2.36 -3.08 -6.27 0.25

💡 Note: The % column shows the percentage of members that CWNU 2479 shares with each listed object.

Visualization

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