CWNU 2584

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0.54 UTI
0.44
CN
1.0
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 3.8 [arcmin]
  • CN 0.44 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 2584 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, near 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)
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 – 280.757 -2.496 0.396 -0.057 -0.363 23.28
Hunt & Reffert 2024 280.729 -2.5 0.387 -0.04 -0.346 34.186
Cavallo et al. 2024 280.756 -2.499 0.398 – – –
Hunt & Reffert 2023 280.729 -2.5 0.387 -0.04 -0.346 34.186
He et al. 2023 280.742 -2.507 0.416 -0.052 -0.354 19.05

💡 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 – – – – – 522* – –
Cavallo et al. 2024 1.71 3.65 – 43 -0.260 – – –
Hunt & Reffert 2023 2.24 3.37 1.88 47 – – – –
He et al. 2023 2.14 3.30 – 126 – – – –

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

Visualization

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