CWNU 1266

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0.30 UTI
0.25
CN
0.26
Cdens
0.5
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 14.9 [arcmin]
  • CN 0.25 Poorly populated
  • Cdens 0.26 Loose
  • CC3 0.5 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 1266 is a poorly populated, loose object of intermediate C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a low-mass, near-solar metallicity, young cluster (see Parameters). It is poorly studied in the literature.
Close Moderate extinction Low mass 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 – 35.987 62.414 0.991 -0.031 -1.781 -27.974
Hunt & Reffert 2024 35.941 62.402 0.978 -0.071 -1.776 -28.291
Cavallo et al. 2024 36.069 62.581 0.983 – – –
Hunt & Reffert 2023 35.941 62.402 0.978 -0.071 -1.776 -28.291
He et al. 2022 36.255 62.365 1.009 -0.017 -1.781 –

💡 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 – – – – – 48* – –
Cavallo et al. 2024 1.00 1.58 – 35 -0.330 – – –
Hunt & Reffert 2023 0.97 1.48 0.48 38 – – – –
He et al. 2022 – 1.50 – 89 – – – –

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

Visualization

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