CWNU 2884

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0.31 UTI
0.0
CN
0.3
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 6.7 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.3 Loose
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 2884 is a sparse, loose object of high C3 quality. Its parallax locates it at a relatively close distance, above 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)
Silver sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 270.116 -20.521 0.53 0.335 -1.225 167.39
Hunt & Reffert 2024 270.138 -20.503 0.53 0.324 -1.238 124.056
Cavallo et al. 2024 270.1 -20.557 0.527 – – –
Hunt & Reffert 2023 270.138 -20.503 0.53 0.324 -1.238 124.056
He et al. 2023 270.08 -20.541 0.53 0.362 -1.225 –

💡 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 – – – – – 386* – –
Cavallo et al. 2024 1.85 3.91 – 36 0.410 – – –
Hunt & Reffert 2023 1.75 3.76 2.75 8 – – – –
He et al. 2023 1.78 2.60 – 1 – – – –

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

Visualization

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