CWNU 1797

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0.46 UTI
0.31
CN
1.0
Cdens
0.5
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 40.4 [N/pc2]
  • CN 0.31 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.5 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 1797 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by very high 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.

Cavallo et al. (2024)
Bronze 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– 262.995 -35.659 0.365 -1.184 -2.986 -15.442
Hunt & Reffert 2024 262.997 -35.659 0.354 -1.165 -2.992 28.254
Cavallo et al. 2024 263.007 -35.655 0.358 – – –
Hunt & Reffert 2023 262.997 -35.659 0.354 -1.165 -2.992 28.254
He et al. 2023 262.99 -35.658 0.381 -1.171 -2.983 –

💡 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– 2.55 5.25 1.9 89 0.140 966 – –
Hunt & Reffert 2024 – – – – – 966(1) – –
Cavallo et al. 2024 3.09 4.92 – 52 0.140 – – –
Hunt & Reffert 2023 2.55 5.40 1.90 89 – – – –
He et al. 2023 2.24 5.25 – 447 – – – –

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

Visualization

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