CWNU 2543

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0.65 UTI
0.76
CN
1.0
Cdens
1.0
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 2.5 [arcmin]
  • CN 0.76 Rich
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 2543 is a rich, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by very high extinction. It is catalogued as a massive, near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age parameter (see Parameters). It was recently reported in the literature.

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

Relatively close Very high extinction Massive Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Wood sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 279.901 -7.043 0.287 0.023 -1.985 28.71
Hunt & Reffert 2024 279.903 -7.039 0.291 0.018 -2.001 43.004
Cavallo et al. 2024 279.898 -7.038 0.29 – – –
Hunt & Reffert 2023 279.903 -7.039 0.291 0.018 -2.001 43.004
He et al. 2023 279.897 -7.035 0.3 0.028 -1.991 28.04

💡 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
Hunt & Reffert 2024 – – – – – 4670* – –
Cavallo et al. 2024 3.52 5.20 – 65 -0.260 – – –
Hunt & Reffert 2023 2.96 4.63 3.17 274 – – – –
He et al. 2023 2.88 5.60 – 282 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
HSC 245 15.1 279.9 -7.05 0.35 0.01 -1.95 26.09 0.08

💡 Note: The % column shows the percentage of members that CWNU 2543 shares with each listed object.

Visualization

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