CWNU 1774

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0.30 UTI
0.31
CN
0.34
Cdens
0.38
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 1.7 [N/pc2]
  • CN 0.31 Poorly populated
  • Cdens 0.34 Loose
  • CC3 0.38 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 1774 is a poorly populated, loose object of low C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a metal-rich, 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 object shares a large percentage of members with a later reported entry. See table with shared members information.

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 99999– 345.475 60.36 0.298 -4.011 -2.544 -70.674
Hunt & Reffert 2024 345.572 60.357 0.293 -3.997 -2.554 –
Cavallo et al. 2024 345.519 60.35 0.296 – – –
Hunt & Reffert 2023 345.572 60.357 0.293 -3.997 -2.554 –
He et al. 2023 345.474 60.336 0.305 -4.016 -2.549 –

💡 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] Bfrac BSS
UCC 99999– 3.24 2.71 1.44 24 0.650 316 – –
Hunt & Reffert 2024 – – – – – 316(1) – –
Cavallo et al. 2024 2.87 2.69 – 76 0.650 – – –
Hunt & Reffert 2023 3.31 2.71 1.44 24 – – – –
He et al. 2023 3.24 3.30 – 11 – – – –

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 2577 77.4 345.5 60.36 0.3 -4.01 -2.54 -70.67 0.05

💡 Note: The % column shows the percentage of members that CWNU 1774 shares with each listed object.

Visualization

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