CWNU 2693

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0.41 UTI
0.36
CN
0.43
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 9.0 [arcmin]
  • CN 0.36 Poorly 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 2693 is a poorly populated, loose object of high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster (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 – 273.553 -18.89 0.643 0.993 -2.643 -12.497
Hunt & Reffert 2024 273.551 -18.886 0.647 0.947 -2.645 -69.814
Cavallo et al. 2024 273.548 -18.863 0.647 – – –
Hunt & Reffert 2023 273.551 -18.886 0.647 0.947 -2.645 -69.814
He et al. 2023 273.546 -18.885 0.653 1.003 -2.628 –

💡 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 – – – – – 130* – –
Cavallo et al. 2024 1.29 1.23 – 45 -0.250 – – –
Hunt & Reffert 2023 1.46 1.22 1.20 57 – – – –
He et al. 2023 1.51 1.45 – 32 – – – –

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

Visualization

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