CWNU 1816

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0.33 UTI
0.28
CN
0.22
Cdens
0.62
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 7.1 [arcmin]
  • CN 0.28 Poorly populated
  • Cdens 0.22 Very loose
  • CC3 0.62 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 1816 is a poorly populated, very loose 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, young cluster, but with a large variance across recent sources for the age parameter (see Parameters). It was recently reported in the literature.
Relatively close Moderate extinction Near-solar metallicity 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 – 156.21 -57.296 0.411 -5.839 2.249 –
Hunt & Reffert 2024 156.192 -57.278 0.411 -5.839 2.246 –
Cavallo et al. 2024 156.256 -57.322 0.411 – – –
Hunt & Reffert 2023 156.192 -57.278 0.411 -5.839 2.246 –
He et al. 2023 156.259 -57.314 0.415 -5.839 2.251 –

💡 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 – – – – – 192* – –
Cavallo et al. 2024 2.22 1.01 – 468 0.020 – – –
Hunt & Reffert 2023 2.24 1.22 2.30 84 – – – –
He et al. 2023 2.29 1.40 – 79 – – – –

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

Visualization

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