CWNU 2877

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0.38 UTI
0.0
CN
1.0
Cdens
0.38
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 1.7 [arcmin]
  • CN 0.0 Sparse
  • Cdens 1.0 Very dense
  • CC3 0.38 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 2877 is a sparse, 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 near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.
Relatively close High extinction Near-solar metallicity 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 – 235.092 -56.256 0.348 -3.803 -3.005 -17.378
Hunt & Reffert 2024 235.083 -56.261 0.344 -3.808 -3.035 -17.603
Cavallo et al. 2024 235.083 -56.258 0.345 – – –
Hunt & Reffert 2023 235.083 -56.261 0.344 -3.808 -3.035 -17.603
He et al. 2023 235.087 -56.264 0.347 -3.798 -3.001 -17.59

💡 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 3.36 4.45 – 224 -0.450 – – –
Hunt & Reffert 2023 2.66 4.35 1.89 138 – – – –
He et al. 2023 2.95 6.30 – 1 – – – –

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

Visualization

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