CWNU 1674

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0.20 UTI
0.31
CN
0.25
Cdens
0.38
CC3
0.25
Clit
0.71
Cdup
Radius (P>50% members) 8.8 [arcmin]
  • CN 0.31 Poorly populated
  • Cdens 0.25 Loose
  • CC3 0.38 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 0.71 Likely unique

Overview

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CWNU 1674 is a poorly populated, loose object of low 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, but with a large variance across recent sources for the age parameter (see Parameters). It was recently reported in the literature.

Note: This is likely a unique object, which shares a moderate percentage of members with at least one previously reported entry. See table with shared members information.

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 – 211.375 -62.033 0.517 -3.669 -2.967 91.423
Hunt & Reffert 2024 211.356 -62.037 0.524 -3.692 -2.935 91.421
Cavallo et al. 2024 211.177 -62.082 0.528 – – –
Hunt & Reffert 2023 211.356 -62.037 0.524 -3.692 -2.935 91.421
He et al. 2023 211.435 -62.007 0.517 -3.642 -2.978 91.42

💡 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 – – – – – 135* – –
Cavallo et al. 2024 1.85 1.39 – 302 0.330 – – –
Hunt & Reffert 2023 1.79 1.73 2.35 80 – – – –
He et al. 2023 2.09 0.55 – 2 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
LS 145 29.0 211.93 -61.91 0.51 -3.67 -3.03 – 0.11

💡 Note: The % column shows the percentage of members that CWNU 1674 shares with each listed object.

Visualization

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