CWNU 2012

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0.36 UTI
0.25
CN
0.3
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 2.5 [arcmin]
  • CN 0.25 Poorly populated
  • Cdens 0.3 Loose
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 2012 is a poorly populated, loose object of high C3 quality. Its parallax locates it at a large distance, near the mid-plane, affected by moderate extinction. It is catalogued as a massive, metal-rich, young cluster (see Parameters). It was recently reported in the literature.
Distant Moderate extinction Massive Metal-rich 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 – 102.464 -0.17 0.178 -0.302 0.502 –
Hunt & Reffert 2024 102.46 -0.174 0.172 -0.301 0.468 79.609
Cavallo et al. 2024 102.446 -0.153 0.17 – – –
Hunt & Reffert 2023 102.46 -0.174 0.172 -0.301 0.468 79.609
He et al. 2023 102.462 -0.172 0.176 -0.34 0.509 –

💡 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 – – – – – 1046* – –
Cavallo et al. 2024 4.51 1.98 – 138 0.800 – – –
Hunt & Reffert 2023 4.88 2.21 2.45 60 – – – –
He et al. 2023 7.94 2.95 – 2 – – – –

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

Visualization

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