CWNU 2651

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0.34 UTI
0.26
CN
0.42
Cdens
0.5
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 4.0 [arcmin]
  • CN 0.26 Poorly populated
  • Cdens 0.42 Loose
  • CC3 0.5 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 2651 is a poorly populated, loose 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 near-solar metallicity, very young cluster (see Parameters). It was recently reported in the literature.
Distant High extinction Near-solar metallicity Very young

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 – 347.218 59.404 0.331 -3.673 -2.925 –
Hunt & Reffert 2024 347.219 59.404 0.327 -3.683 -2.924 –
Cavallo et al. 2024 347.185 59.429 0.326 – – –
Hunt & Reffert 2023 347.219 59.404 0.327 -3.683 -2.924 –
He et al. 2023 347.217 59.41 0.345 -3.692 -2.918 –

💡 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 – – – – – 892* – –
Cavallo et al. 2024 3.48 3.58 – 27 0.490 – – –
Hunt & Reffert 2023 2.84 3.52 2.65 5 – – – –
He et al. 2023 3.31 4.35 – 5 – – – –

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

Visualization

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