CWNU 2554

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0.31 UTI
0.76
CN
1.0
Cdens
0.75
CC3
0.25
Clit
0.52
Cdup
Radius (P>50% members) 4.7 [arcmin]
  • CN 0.76 Rich
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 0.52 Likely unique

Overview

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CWNU 2554 is a rich, very dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.

Note: This is likely a unique object, which shares a moderate percentage of members with at least one previously reported entry. See table with shared members information.

Relatively close Moderate 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 – 160.452 -58.384 0.322 -6.494 3.454 -10.001
Hunt & Reffert 2024 160.462 -58.374 0.318 -6.482 3.444 -13.318
Cavallo et al. 2024 160.472 -58.391 0.318 – – –
Hunt & Reffert 2023 160.462 -58.374 0.318 -6.482 3.444 -13.318
He et al. 2023 160.451 -58.373 0.327 -6.492 3.458 -13.17

💡 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 – – – – – 637* – –
Cavallo et al. 2024 3.25 1.65 – 56 0.410 – – –
Hunt & Reffert 2023 2.80 1.53 2.52 167 – – – –
He et al. 2023 2.82 2.00 – 71 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
FoF 1487 47.9 160.5 -58.39 0.31 -6.53 3.41 4.27 0.47

💡 Note: The % column shows the percentage of members that CWNU 2554 shares with each listed object.

Visualization

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