CWNU 2739

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0.44 UTI
0.53
CN
0.43
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 7.3 [arcmin]
  • CN 0.53 Moderately populated
  • Cdens 0.43 Loose
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 2739 is a moderately populated, loose object of high C3 quality. Its parallax locates it at a moderate distance, below 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 parameter (see Parameters). It was recently reported in the literature.
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 – 324.454 48.544 0.417 -3.672 -3.734 -65.923
Hunt & Reffert 2024 324.531 48.605 0.4 -3.636 -3.734 -71.55
Cavallo et al. 2024 324.479 48.565 0.412 – – –
Hunt & Reffert 2023 324.531 48.605 0.4 -3.636 -3.734 -71.55
He et al. 2023 324.454 48.547 0.427 -3.665 -3.741 –

💡 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 – – – – – 319* – –
Cavallo et al. 2024 2.09 1.41 – 19 -0.260 – – –
Hunt & Reffert 2023 2.28 1.13 2.44 128 – – – –
He et al. 2023 2.24 1.40 – 28 – – – –

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

Visualization

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