CWNU 1673

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0.35 UTI
0.0
CN
0.49
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 2.8 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.49 Loose
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 1673 is a sparse, loose object of high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.
Distant High 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 – 145.484 -56.288 0.278 -5.503 4.514 8.196
Hunt & Reffert 2024 145.494 -56.316 0.285 -5.496 4.523 8.137
Cavallo et al. 2024 145.487 -56.3 0.282 – – –
Hunt & Reffert 2023 145.494 -56.316 0.285 -5.496 4.523 8.137
He et al. 2023 145.485 -56.297 0.277 -5.506 4.514 19.22

💡 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 – – – – – 858* – –
Cavallo et al. 2024 3.56 3.62 – 204 0.150 – – –
Hunt & Reffert 2023 3.21 3.32 2.44 280 – – – –
He et al. 2023 3.24 3.40 – 562 – – – –

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

Visualization

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