CWNU 2470

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0.35 UTI
0.0
CN
0.74
Cdens
0.5
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 4.5 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.74 Moderately dense
  • CC3 0.5 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 2470 is a sparse, moderately dense object of intermediate C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It was recently reported in the literature.
Relatively close High extinction Near-solar metallicity Very young

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 – 275.889 -13.317 0.537 0.725 -0.212 -50.653
Hunt & Reffert 2024 275.886 -13.311 0.542 0.75 -0.215 -50.65
Cavallo et al. 2024 275.889 -13.338 0.54 – – –
Hunt & Reffert 2023 275.886 -13.311 0.542 0.75 -0.215 -50.65
He et al. 2023 275.881 -13.309 0.539 0.754 -0.215 –

💡 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 – – – – – 284* – –
Cavallo et al. 2024 1.60 3.21 – 58 -0.050 – – –
Hunt & Reffert 2023 1.76 3.21 2.19 9 – – – –
He et al. 2023 1.70 0.80 – 1 – – – –

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

Visualization

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