CWNU 1451

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0.44 UTI
0.49
CN
0.56
Cdens
0.5
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members) 7.4 [arcmin]
  • CN 0.49 Poorly populated
  • Cdens 0.56 Moderately dense
  • CC3 0.5 Intermediate quality
  • Clit 0.31 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 1451 is a poorly populated, moderately dense object of intermediate C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.
Relatively close Moderate 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 – 90.08 24.43 0.516 1.914 -2.792 -11.401
Zhang et al. 2024 90.067 24.406 – – – –
Hunt & Reffert 2024 90.067 24.406 0.52 1.92 -2.794 -11.365
Cavallo et al. 2024 90.068 24.453 0.523 – – –
Hunt & Reffert 2023 90.067 24.406 0.52 1.92 -2.794 -11.365
He et al. 2023 90.073 24.433 0.522 1.914 -2.789 -11.4

💡 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 – – – – -0.045* – – –
Hunt & Reffert 2024 – – – – – 262* – –
Cavallo et al. 2024 1.81 1.92 – 490 0.120 – – –
Hunt & Reffert 2023 1.81 1.83 1.42 422 – – – –
He et al. 2023 1.78 1.80 – 794 – – – –

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

Visualization

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