CWNU 134

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0.39 UTI
0.26
CN
0.54
Cdens
0.5
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members) 9.0 [arcmin]
  • CN 0.26 Poorly populated
  • Cdens 0.54 Moderately dense
  • CC3 0.5 Intermediate quality
  • Clit 0.31 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 134 is a poorly populated, moderately dense object of intermediate C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is poorly studied in the literature.
Relatively close Low extinction Near-solar metallicity Intermediate age

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 – 296.285 19.012 0.845 -0.884 -4.397 -1.708
Hunt & Reffert 2024 296.259 18.998 0.831 -0.902 -4.415 3.096
Cavallo et al. 2024 296.307 19.036 0.836 – – –
Hunt & Reffert 2023 296.259 18.998 0.831 -0.902 -4.415 3.096
He et al. 2022 296.299 19.034 0.838 -0.879 -4.39 –
He et al. 2022 296.287 19.009 0.81 -0.88 -4.39 –

💡 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 – – – – – 115* – –
Cavallo et al. 2024 1.31 1.11 – 182 0.190 – – –
Hunt & Reffert 2023 1.16 0.86 0.38 173 – – – –
He et al. 2022 – 1.15 – 355 – – – –
He et al. 2022 1.05 0.78 – 316 0.274 – – –

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

Visualization

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