CWNU 301

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0.46 UTI
0.52
CN
0.67
Cdens
0.62
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 10.4 [arcmin]
  • CN 0.52 Moderately populated
  • Cdens 0.67 Moderately dense
  • CC3 0.62 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 301 is a moderately populated, moderately dense object of intermediate C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is poorly studied in the literature.
Relatively close Low 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 – 125.75 -31.659 0.759 -4.956 4.347 19.887
Hunt & Reffert 2024 125.698 -31.616 0.753 -4.944 4.347 25.088
Cavallo et al. 2024 125.766 -31.622 0.76 – – –
Hunt & Reffert 2023 125.698 -31.616 0.753 -4.944 4.347 25.088
He et al. 2022 125.764 -31.625 0.75 -4.96 4.32 –

💡 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 – – – – – 110* – –
Cavallo et al. 2024 1.34 0.41 – 51 0.030 – – –
Hunt & Reffert 2023 1.27 0.24 0.56 51 – – – –
He et al. 2022 1.20 0.48 – 32 -0.236 – – –

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

Visualization

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