CWNU 2842

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0.29 UTI
0.0
CN
0.7
Cdens
0.25
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 2.8 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.7 Moderately dense
  • CC3 0.25 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 2842 is a sparse, moderately 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.
Distant 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 – 63.68 50.367 0.31 0.756 -1.027 –
Hunt & Reffert 2024 63.677 50.368 0.312 0.761 -1.039 –
Cavallo et al. 2024 63.652 50.365 0.308 – – –
Hunt & Reffert 2023 63.677 50.368 0.312 0.761 -1.039 –
He et al. 2023 63.72 50.341 0.299 0.762 -1.025 -56.76

💡 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 – – – – – 230* – –
Cavallo et al. 2024 3.45 3.44 – 115 0.100 – – –
Hunt & Reffert 2023 2.94 2.98 1.44 208 – – – –
He et al. 2023 3.39 3.20 – 794 – – – –

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

Visualization

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