CWNU 2606

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0.53 UTI
0.41
CN
1.0
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 5.2 [arcmin]
  • CN 0.41 Poorly 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 2606 is a poorly 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, young cluster (see Parameters). It was recently reported in the literature.
Relatively close Moderate extinction Near-solar metallicity 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 – 257.85 -41.757 0.651 1.071 -2.217 -44.122
Hunt & Reffert 2024 257.884 -41.749 0.626 1.082 -2.246 -44.128
Cavallo et al. 2024 257.866 -41.753 0.632 – – –
Hunt & Reffert 2023 257.884 -41.749 0.626 1.082 -2.246 -44.128
He et al. 2023 257.867 -41.739 0.658 1.05 -2.213 –

💡 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 – – – – – 308* – –
Cavallo et al. 2024 1.44 2.16 – 37 -0.010 – – –
Hunt & Reffert 2023 1.46 2.11 1.93 58 – – – –
He et al. 2023 1.45 2.15 – 25 – – – –

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

Visualization

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