CWNU 2713

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0.43 UTI
0.48
CN
0.18
Cdens
1.0
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 6.2 [arcmin]
  • CN 0.48 Poorly populated
  • Cdens 0.18 Very loose
  • CC3 1.0 Very high quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 2713 is a poorly populated, very loose object of very high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by high extinction. It is catalogued as a massive, metal-rich, young cluster (see Parameters). It was recently reported in the literature.
Distant High extinction Massive Metal-rich 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 – 293.395 17.48 0.25 -3.001 -6.295 14.986
Hunt & Reffert 2024 293.399 17.418 0.245 -2.997 -6.299 –
Cavallo et al. 2024 293.384 17.481 0.249 – – –
Hunt & Reffert 2023 293.399 17.418 0.245 -2.997 -6.299 –
He et al. 2023 293.421 17.497 0.257 -2.995 -6.298 14.99

💡 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 – – – – – 1616* – –
Cavallo et al. 2024 4.43 4.42 – 28 0.610 – – –
Hunt & Reffert 2023 3.67 4.67 2.39 28 – – – –
He et al. 2023 4.68 5.30 – 2 – – – –

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

Visualization

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