CWNU 1637

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0.52 UTI
0.33
CN
1.0
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 2.4 [arcmin]
  • CN 0.33 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 1637 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.
Relatively close Moderate 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 – 220.341 -57.653 0.479 -3.201 -2.797 -38.083
Hunt & Reffert 2024 220.344 -57.65 0.482 -3.196 -2.775 –
Cavallo et al. 2024 220.338 -57.647 0.482 – – –
Hunt & Reffert 2023 220.344 -57.65 0.482 -3.196 -2.775 –
He et al. 2023 220.341 -57.647 0.489 -3.228 -2.799 –

💡 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 – – – – – 250* – –
Cavallo et al. 2024 1.75 1.78 – 141 0.160 – – –
Hunt & Reffert 2023 1.94 1.71 1.09 136 – – – –
He et al. 2023 1.91 2.20 – 40 – – – –

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

Visualization

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