CWNU 70

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0.58 UTI
0.64
CN
1.0
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 4.6 [arcmin]
  • CN 0.64 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 70 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a massive, near-solar metallicity, young cluster (see Parameters). It is poorly studied in the literature.
Relatively close High extinction Massive 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 – 277.959 -10.107 0.434 0.583 -1.41 30.286
Hunt & Reffert 2024 277.963 -10.145 0.439 0.57 -1.38 98.712
Cavallo et al. 2024 277.957 -10.123 0.435 – – –
Hunt & Reffert 2023 277.963 -10.145 0.439 0.57 -1.38 98.712
He et al. 2022 277.945 -10.101 0.43 0.63 -1.46 31.8

💡 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 – – – – – 1012* – –
Cavallo et al. 2024 2.10 4.10 – 89 0.040 – – –
Hunt & Reffert 2023 2.03 4.55 2.69 52 – – – –
He et al. 2022 1.66 3.96 – 1000 -0.642 – – –

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

Visualization

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