CWNU 1313

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0.39 UTI
0.53
CN
0.31
Cdens
0.38
CC3
0.38
Clit
1.0
Cdup
Radius (P>50% members) 8.3 [arcmin]
  • CN 0.53 Moderately populated
  • Cdens 0.31 Loose
  • CC3 0.38 Low quality
  • Clit 0.38 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 1313 is a moderately populated, loose object of low 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, but with a large variance across recent sources for the metallicity parameter (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 – 94.965 1.936 0.404 0.524 -2.396 52.084
Hu & Soubiran 2025 94.91 1.924 – – – –
Zhang et al. 2024 94.997 1.923 – – – –
Hunt & Reffert 2024 94.997 1.923 0.394 0.508 -2.371 39.241
Cavallo et al. 2024 94.91 1.924 0.393 – – –
Hunt & Reffert 2023 94.997 1.923 0.394 0.508 -2.371 39.241
He et al. 2023 94.969 1.917 0.418 0.522 -2.423 52.08

💡 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
Hu & Soubiran 2025 – – – – -0.190* – – –
Zhang et al. 2024 – – – – 0.032* – – –
Hunt & Reffert 2024 – – – – – 142* – –
Cavallo et al. 2024 2.33 1.35 – 631 0.140 – – –
Hunt & Reffert 2023 2.26 1.18 0.91 489 – – – –
He et al. 2023 2.29 1.50 – 794 – – – –

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

Visualization

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