CWNU 1

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0.00 UTI
0.32
CN
0.53
Cdens
0.75
CC3
0.0
Clit
0.0
Cdup
Core radius and density 1.2 [pc], 2.6 [pc-2]
  • CN 0.32 Poorly populated
  • Cdens 0.53 Moderately dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 0.0 Very likely duplicate

Overview

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CWNU 1 is a poorly populated, moderately dense object of high C3 quality. Its parallax locates it at a relatively close distance, near 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 age 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– 259.266 -41.693 0.6 -0.04 -3.595 -30.225
Li et al. 2023 259.264 -41.687 0.59 -0.05 -3.58 –
He et al. 2022 259.257 -41.692 0.6 -0.03 -3.58 -18.1

💡 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– 1.805 2.75 – 730 -0.254 – – 1
Li et al. 2023 2.29 2.20 – 1259 -0.228 – – 1(1)
He et al. 2022 1.32 3.30 – 200 -0.279 – – –

(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 1563 100.0 259.26 -41.7 0.6 -0.05 -3.59 -30.23 0.51
CWWDL 13348 84.4 259.26 -41.7 0.6 -0.03 -3.59 -39.28 0.0

💡 Note: The % column shows the percentage of members that CWNU 1 shares with each listed object.

Visualization

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