CWNU 1914

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0.27 UTI
0.0
CN
0.22
Cdens
0.62
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 7.6 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.22 Very loose
  • CC3 0.62 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 1914 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.
Relatively close Low extinction Near-solar metallicity Young

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 – 132.489 -54.596 0.469 -5.427 4.611 -25.716
Hunt & Reffert 2024 132.534 -54.576 0.465 -5.441 4.637 -25.81
Cavallo et al. 2024 132.53 -54.566 0.467 – – –
Hunt & Reffert 2023 132.534 -54.576 0.465 -5.441 4.637 -25.81
He et al. 2023 132.496 -54.583 0.469 -5.427 4.615 –

💡 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 – – – – – 165* – –
Cavallo et al. 2024 1.95 1.01 – 52 -0.270 – – –
Hunt & Reffert 2023 1.99 0.60 0.72 168 – – – –
He et al. 2023 2.04 0.85 – 79 – – – –

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

Visualization

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