CWNU 2619

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0.61 UTI
0.54
CN
1.0
Cdens
1.0
CC3
0.31
Clit
0.96
Cdup
Radius (P>50% members) 1.8 [arcmin]
  • CN 0.54 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.31 Poorly studied
  • Cdup 0.96 Unique

Overview

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CWNU 2619 is a moderately populated, very dense object of very 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, but with a large variance across recent sources for the age and metallicity parameters (see Parameters). It was recently reported in the literature.

Note: This is a unique object, which shares a very small 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 – 314.902 44.964 0.321 -3.571 -4.559 -27.32
Zhang et al. 2024 314.901 44.97 – – – –
Hunt & Reffert 2024 314.901 44.97 0.317 -3.57 -4.551 -27.336
Cavallo et al. 2024 314.891 44.955 0.316 – – –
Hunt & Reffert 2023 314.901 44.97 0.317 -3.57 -4.551 -27.336
He et al. 2023 314.903 44.967 0.326 -3.57 -4.558 –

💡 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
Zhang et al. 2024 – – – – -0.221* – – –
Hunt & Reffert 2024 – – – – – 383* – –
Cavallo et al. 2024 2.95 1.92 – 380 0.130 – – –
Hunt & Reffert 2023 2.90 1.96 1.56 97 – – – –
He et al. 2023 3.24 2.45 – 16 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
FoF 341 3.5 314.9 44.93 0.27 -3.4 -4.4 -33.82 0.03

💡 Note: The % column shows the percentage of members that CWNU 2619 shares with each listed object.

Visualization

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