CWNU 455

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0.41 UTI
0.31
CN
0.5
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 9.4 [arcmin]
  • CN 0.31 Poorly populated
  • Cdens 0.5 Moderately dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 455 is a poorly populated, moderately dense object of high C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is poorly studied in the literature.
Relatively close High extinction Near-solar metallicity Young

Cavallo et al. (2024)
Bronze sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 304.831 41.378 0.775 -2.424 -3.03 -14.04
Hunt & Reffert 2024 304.843 41.4 0.776 -2.444 -3.102 -32.188
Cavallo et al. 2024 304.815 41.256 0.776 – – –
Hunt & Reffert 2023 304.843 41.4 0.776 -2.444 -3.102 -32.188
He et al. 2022 304.827 41.38 0.78 -2.38 -3.02 –

💡 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 – – – – – 152* – –
Cavallo et al. 2024 1.73 3.31 – 20 0.520 – – –
Hunt & Reffert 2023 1.25 3.35 2.42 18 – – – –
He et al. 2022 1.02 3.72 – 20 -0.930 – – –

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

Visualization

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