CWNU 2712

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0.38 UTI
0.28
CN
0.39
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 6.8 [arcmin]
  • CN 0.28 Poorly populated
  • Cdens 0.39 Loose
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 2712 is a poorly populated, loose object of high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.
Relatively close Low extinction Near-solar metallicity Intermediate age

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 – 174.688 -60.686 0.524 -8.651 1.138 -0.287
Hunt & Reffert 2024 174.693 -60.691 0.527 -8.647 1.127 -0.291
Cavallo et al. 2024 174.617 -60.697 0.524 – – –
Hunt & Reffert 2023 174.693 -60.691 0.527 -8.647 1.127 -0.291
He et al. 2023 174.691 -60.684 0.526 -8.645 1.137 –

💡 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
Hunt & Reffert 2024 – – – – – 120* – –
Cavallo et al. 2024 1.57 1.02 – 407 -0.330 – – –
Hunt & Reffert 2023 1.80 0.79 0.57 392 – – – –
He et al. 2023 1.78 0.90 – 40 – – – –

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

Visualization

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