CWNU 87

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0.42 UTI
0.32
CN
0.43
Cdens
0.75
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members) 4.3 [arcmin]
  • CN 0.32 Poorly populated
  • Cdens 0.43 Loose
  • CC3 0.75 High quality
  • Clit 0.31 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 87 is a poorly populated, loose 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 is poorly studied in the literature.

Note: This object shares a significant percentage of members with a later reported entry. See table with shared members information.

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 – 22.617 59.633 0.322 -1.181 -0.707 -52.7
Zhang et al. 2024 22.613 59.633 – – – –
Hunt & Reffert 2024 22.613 59.633 0.32 -1.197 -0.667 -52.685
Cavallo et al. 2024 22.683 59.659 0.32 – – –
Hunt & Reffert 2023 22.613 59.633 0.32 -1.197 -0.667 -52.685
He et al. 2022 22.611 59.641 0.33 -1.18 -0.71 -53.3

💡 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 – – – – -0.240* – – –
Hunt & Reffert 2024 – – – – – 223* – –
Cavallo et al. 2024 2.41 1.49 – 68 0.050 – – –
Hunt & Reffert 2023 2.79 1.38 0.55 206 – – – –
He et al. 2022 2.40 1.86 – 251 -2.028 – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 4624 62.5 22.59 59.63 0.32 -1.19 -0.66 7.92 0.04

💡 Note: The % column shows the percentage of members that CWNU 87 shares with each listed object.

Visualization

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