CWNU 1899

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0.45 UTI
0.0
CN
1.0
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 1.7 [arcmin]
  • CN 0.0 Sparse
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 1899 is a sparse, very dense object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by high extinction. It is catalogued as a very metal-rich, very young cluster (see Parameters). It was recently reported in the literature.
Distant High extinction Very metal-rich 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 – 58.05 54.507 0.232 -0.225 -0.343 –
Hunt & Reffert 2024 58.041 54.494 0.243 -0.23 -0.342 –
Cavallo et al. 2024 58.063 54.506 0.243 – – –
Hunt & Reffert 2023 58.041 54.494 0.243 -0.23 -0.342 –
He et al. 2023 58.063 54.509 0.246 -0.225 -0.365 –

💡 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 – – – – – 425* – –
Cavallo et al. 2024 3.52 3.00 – 91 1.140 – – –
Hunt & Reffert 2023 3.84 3.61 0.94 18 – – – –
He et al. 2023 3.89 4.05 – 6 – – – –

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

Visualization

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