CWNU 356

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0.55 UTI
0.52
CN
1.0
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 4.4 [arcmin]
  • CN 0.52 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 356 is a moderately populated, very dense object of high 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, very young cluster (see Parameters). It is poorly studied in the literature.
Relatively close Moderate extinction Near-solar metallicity Very 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 – 215.066 -61.074 0.572 -3.704 -2.898 6.882
Hunt & Reffert 2024 215.058 -61.081 0.584 -3.673 -2.888 6.953
Cavallo et al. 2024 215.094 -61.057 0.585 – – –
Hunt & Reffert 2023 215.058 -61.081 0.584 -3.673 -2.888 6.953
He et al. 2022 215.061 -61.073 0.57 -3.71 -2.9 –

💡 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 – – – – – 302* – –
Cavallo et al. 2024 1.62 1.21 – 17 -0.030 – – –
Hunt & Reffert 2023 1.60 1.49 1.20 6 – – – –
He et al. 2022 2.19 1.80 – 5 0.680 – – –

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

Visualization

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