CWNU 2719

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0.63 UTI
0.66
CN
1.0
Cdens
1.0
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 2.5 [arcmin]
  • CN 0.66 Moderately populated
  • 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 2719 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 high extinction. It is catalogued as a massive, metal-poor, 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 large percentage of members with a later reported entry. See table with shared members information.

Relatively close High extinction Massive Metal-poor Intermediate age

Cavallo et al. (2024)
Silver sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 274.598 -19.361 0.491 -0.694 -0.049 -22.418
Hunt & Reffert 2024 274.593 -19.36 0.473 -0.694 -0.082 -17.475
Cavallo et al. 2024 274.625 -19.33 0.476 – – –
Hunt & Reffert 2023 274.593 -19.36 0.473 -0.694 -0.082 -17.475
He et al. 2023 274.602 -19.348 0.499 -0.696 -0.045 -22.18

💡 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 – – – – – 1497* – –
Cavallo et al. 2024 1.86 3.15 – 1820 -0.660 – – –
Hunt & Reffert 2023 1.89 3.50 2.36 353 – – – –
He et al. 2023 2.24 1.90 – 1 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 969 82.7 274.6 -19.36 0.49 -0.69 -0.05 -22.42 0.0

💡 Note: The % column shows the percentage of members that CWNU 2719 shares with each listed object.

Visualization

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