CWNU 2745

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0.51 UTI
0.56
CN
1.0
Cdens
0.5
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 2.4 [arcmin]
  • CN 0.56 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 0.5 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 2745 is a moderately populated, very dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a massive, 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.
Distant High extinction Massive 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 – 183.397 -63.023 0.226 -6.708 0.28 –
Hunt & Reffert 2024 183.391 -63.028 0.222 -6.714 0.267 –
Cavallo et al. 2024 183.374 -63.016 0.222 – – –
Hunt & Reffert 2023 183.391 -63.028 0.222 -6.714 0.267 –
He et al. 2023 183.389 -63.029 0.245 -6.704 0.283 –

💡 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 – – – – – 1140* – –
Cavallo et al. 2024 3.78 3.37 – 145 0.410 – – –
Hunt & Reffert 2023 3.99 3.47 2.48 27 – – – –
He et al. 2023 3.98 4.05 – 6 – – – –

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

Visualization

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