CWNU 2006

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0.29 UTI
0.0
CN
0.33
Cdens
0.62
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 7.4 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.33 Loose
  • CC3 0.62 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 2006 is a sparse, loose object of intermediate C3 quality. Its parallax locates it at a relatively close distance, above 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 – 113.645 -17.168 0.607 -3.251 0.983 –
Hunt & Reffert 2024 113.581 -17.187 0.608 -3.271 1.009 –
Cavallo et al. 2024 113.612 -17.141 0.608 – – –
Hunt & Reffert 2023 113.581 -17.187 0.608 -3.271 1.009 –
He et al. 2023 113.646 -17.144 0.606 -3.251 0.986 –

💡 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 – – – – – 79* – –
Cavallo et al. 2024 1.52 0.51 – 427 -0.010 – – –
Hunt & Reffert 2023 1.53 0.30 1.11 486 – – – –
He et al. 2023 1.58 0.80 – 50 – – – –

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

Visualization

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