CWNU 15

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0.25 UTI
0.0
CN
0.11
Cdens
0.5
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members) 19.6 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.11 Very loose
  • CC3 0.5 Intermediate quality
  • Clit 0.31 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 15 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It is poorly studied in the literature.
Relatively close Low 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 – 87.409 26.122 0.861 -0.396 -2.685 1.683
Zhang et al. 2024 87.526 26.137 – – – –
Hunt & Reffert 2024 87.526 26.137 0.863 -0.401 -2.632 11.537
Cavallo et al. 2024 87.464 25.982 0.863 – – –
Hunt & Reffert 2023 87.526 26.137 0.863 -0.401 -2.632 11.537
He et al. 2022 87.48 26.166 0.88 -0.39 -2.7 –

💡 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
Zhang et al. 2024 – – – – -0.049* – – –
Hunt & Reffert 2024 – – – – – 60* – –
Cavallo et al. 2024 1.14 0.98 – 132 0.400 – – –
Hunt & Reffert 2023 1.09 0.95 0.75 96 – – – –
He et al. 2022 0.93 1.44 – 32 -2.028 – – –

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

Visualization

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