CWNU 2028

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0.27 UTI
0.0
CN
0.61
Cdens
0.25
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 3.1 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.61 Moderately dense
  • CC3 0.25 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 2028 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, very young cluster, but with a large variance across recent sources for the age parameter (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 – 240.503 -54.039 0.336 -3.24 -4.181 -29.297
Hunt & Reffert 2024 240.525 -54.018 0.327 -3.213 -4.165 32.389
Cavallo et al. 2024 240.593 -53.932 0.329 – – –
Hunt & Reffert 2023 240.525 -54.018 0.327 -3.213 -4.165 32.389
He et al. 2023 240.508 -54.022 0.333 -3.249 -4.183 –

💡 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 – – – – – 471* – –
Cavallo et al. 2024 2.38 3.16 – 126 -0.430 – – –
Hunt & Reffert 2023 2.71 3.20 2.81 18 – – – –
He et al. 2023 3.55 3.90 – 3 – – – –

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

Visualization

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