CWNU 2145

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0.23 UTI
0.0
CN
0.13
Cdens
0.38
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members) 11.1 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.13 Very loose
  • CC3 0.38 Low quality
  • Clit 0.31 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 2145 is a sparse, very loose object of low C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It was recently reported in the literature.
Relatively close Moderate extinction Near-solar metallicity 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 – 83.662 36.432 0.594 1.129 -3.113 –
Zhang et al. 2024 83.413 36.465 – – – –
Hunt & Reffert 2024 83.413 36.465 0.589 1.02 -3.092 -68.392
Cavallo et al. 2024 83.667 36.579 0.595 – – –
Hunt & Reffert 2023 83.413 36.465 0.589 1.02 -3.092 -68.392
He et al. 2023 83.677 36.383 0.622 1.261 -3.137 –

💡 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 – – – – -0.353* – – –
Hunt & Reffert 2024 – – – – – 131* – –
Cavallo et al. 2024 1.84 1.51 – 63 0.560 – – –
Hunt & Reffert 2023 1.61 1.92 2.32 40 – – – –
He et al. 2023 1.74 3.00 – 9 – – – –

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

Visualization

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