CWNU 1780

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0.40 UTI
0.0
CN
1.0
Cdens
0.5
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 3.0 [arcmin]
  • CN 0.0 Sparse
  • 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 1780 is a sparse, very dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It was recently reported in the literature.
Relatively close Moderate extinction Near-solar metallicity Very 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 – 5.709 62.238 0.467 -2.85 -1.628 –
Hunt & Reffert 2024 5.726 62.239 0.467 -2.856 -1.63 –
Cavallo et al. 2024 5.756 62.243 0.467 – – –
Hunt & Reffert 2023 5.726 62.239 0.467 -2.856 -1.63 –
He et al. 2023 5.722 62.239 0.466 -2.847 -1.629 –

💡 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 – – – – – 237* – –
Cavallo et al. 2024 2.04 1.21 – 4 0.020 – – –
Hunt & Reffert 2023 1.99 1.03 0.77 8 – – – –
He et al. 2023 2.09 1.60 – 8 – – – –

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

Visualization

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