CWNU 2038

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0.40 UTI
0.26
CN
0.85
Cdens
0.25
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members) 3.4 [arcmin]
  • CN 0.26 Poorly populated
  • Cdens 0.85 Dense
  • CC3 0.25 Low quality
  • Clit 0.31 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 2038 is a poorly populated, dense object of low C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the absorption, age, and metallicity parameters (see Parameters). It was recently reported in the literature.
Relatively close Low extinction Near-solar metallicity Intermediate age

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 – 109.248 -2.081 0.4 -2.501 1.331 50.508
Zhang et al. 2024 109.253 -2.11 – – – –
Hunt & Reffert 2024 109.253 -2.11 0.38 -2.488 1.324 50.513
Cavallo et al. 2024 109.243 -2.084 0.391 – – –
Hunt & Reffert 2023 109.253 -2.11 0.38 -2.488 1.324 50.513
He et al. 2023 109.233 -2.068 0.396 -2.497 1.318 50.51

💡 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
Zhang et al. 2024 – – – – -0.067* – – –
Hunt & Reffert 2024 – – – – – 76* – –
Cavallo et al. 2024 4.23 1.15 – 41 0.420 – – –
Hunt & Reffert 2023 2.34 0.23 0.36 542 – – – –
He et al. 2023 2.34 0.35 – 398 – – – –

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

Visualization

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