CWNU 365

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0.02 UTI
0.52
CN
0.13
Cdens
0.5
CC3
0.0
Clit
0.07
Cdup
Core radius and density 3.3 [pc], 0.6 [pc-2]
  • CN 0.52 Moderately populated
  • Cdens 0.13 Very loose
  • CC3 0.5 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 0.07 Very likely duplicate

Overview

â„šī¸
CWNU 365 is a moderately populated, very loose object of intermediate C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, old cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It is rarely studied in the literature.

âš ī¸ Warning: This is very likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

Note: This object contains blue stragglers according to at least one source.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 45.496 47.963 0.334 0.523 -1.236 -28.277
Li et al. 2023 45.515 47.964 0.34 0.52 -1.27 –
He et al. 2022 45.503 47.966 0.33 0.49 -1.24 -30.1

💡 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] Bfrac BSS
UCC 99999– 2.575 0.535 – 2048 0.247 – – 1
Li et al. 2023 2.40 0.50 – 2512 0.097 – – 1(1)
He et al. 2022 2.75 0.57 – 1585 0.398 – – –

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
UBC 1246 92.7 45.48 47.96 0.34 0.53 -1.24 -28.68 0.28
OC 0268 43.6 45.49 47.94 0.35 0.51 -1.25 -28.68 0.0

💡 Note: The % column shows the percentage of members that CWNU 365 shares with each listed object.

Visualization

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