CWNU 1664

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0.58 UTI
0.39
CN
1.0
Cdens
1.0
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 1.1 [arcmin]
  • CN 0.39 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 1664 is a poorly populated, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by very high extinction. It is catalogued as a massive, near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.
Distant Very high extinction Massive 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 – 271.856 -21.669 0.287 -1.238 -2.639 -7.305
Hunt & Reffert 2024 271.86 -21.67 0.276 -1.217 -2.614 33.084
Cavallo et al. 2024 271.861 -21.664 0.278 – – –
Hunt & Reffert 2023 271.86 -21.67 0.276 -1.217 -2.614 33.084
He et al. 2023 271.857 -21.659 0.287 -1.232 -2.641 -7.91

💡 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 – – – – – 1758* – –
Cavallo et al. 2024 2.70 4.75 – 234 0.270 – – –
Hunt & Reffert 2023 3.06 5.21 2.55 51 – – – –
He et al. 2023 3.02 5.45 – 141 – – – –

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

Visualization

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