CWNU 1910

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0.36 UTI
0.0
CN
0.53
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 3.2 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.53 Moderately dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 1910 is a sparse, moderately dense object of high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.
Relatively close Moderate extinction Near-solar metallicity Intermediate age

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 – 219.532 -63.396 0.33 -6.899 -4.532 -34.031
Hunt & Reffert 2024 219.544 -63.395 0.329 -6.916 -4.541 -33.91
Cavallo et al. 2024 219.544 -63.388 0.33 – – –
Hunt & Reffert 2023 219.544 -63.395 0.329 -6.916 -4.541 -33.91
He et al. 2023 219.549 -63.397 0.319 -6.907 -4.529 –

💡 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 – – – – – 303* – –
Cavallo et al. 2024 1.99 2.15 – 174 -0.270 – – –
Hunt & Reffert 2023 2.67 1.69 1.83 206 – – – –
He et al. 2023 2.82 2.20 – 56 – – – –

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

Visualization

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