CWNU 1785

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0.46 UTI
0.32
CN
0.5
Cdens
1.0
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 4.1 [arcmin]
  • CN 0.32 Poorly populated
  • Cdens 0.5 Moderately dense
  • CC3 1.0 Very high quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 1785 is a poorly populated, moderately dense object of very high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a massive, very metal-poor, very 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)
Silver 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– 267.847 -27.752 0.334 -0.125 -2.124 -2.481
Hunt & Reffert 2024 267.901 -27.742 0.336 -0.128 -2.14 -6.559
Cavallo et al. 2024 267.87 -27.766 0.335 – – –
Hunt & Reffert 2023 267.901 -27.742 0.336 -0.128 -2.14 -6.559
He et al. 2023 267.864 -27.758 0.333 -0.098 -2.126 -39.69

💡 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– 2.68 3.74 2.61 17 -1.040 1001 – –
Hunt & Reffert 2024 – – – – – 1001(1) – –
Cavallo et al. 2024 2.65 3.74 – 71 -1.040 – – –
Hunt & Reffert 2023 2.68 3.60 2.61 17 – – – –
He et al. 2023 2.69 4.40 – 9 – – – –

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

Visualization

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