CWNU 2621

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0.29 UTI
0.0
CN
0.39
Cdens
0.75
CC3
0.25
Clit
0.88
Cdup
Radius (P>50% members) 3.1 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.39 Loose
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 0.88 Very likely unique

Overview

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CWNU 2621 is a sparse, loose object of high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by very high extinction. It is catalogued as a massive, near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.

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

Distant 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 – 259.774 -42.356 0.262 -0.972 -3.177 -78.012
Hunt & Reffert 2024 259.784 -42.356 0.257 -0.945 -3.167 -60.965
Cavallo et al. 2024 259.758 -42.36 0.255 – – –
Hunt & Reffert 2023 259.784 -42.356 0.257 -0.945 -3.167 -60.965
He et al. 2023 259.772 -42.362 0.272 -0.927 -3.178 -69.45

💡 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 – – – – – 1518* – –
Cavallo et al. 2024 3.56 4.32 – 182 0.470 – – –
Hunt & Reffert 2023 3.30 5.17 2.63 101 – – – –
He et al. 2023 3.02 5.10 – 562 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
VVVX CL056 12.0 259.49 -42.23 0.27 -0.99 -3.15 -52.87 0.05

💡 Note: The % column shows the percentage of members that CWNU 2621 shares with each listed object.

Visualization

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