CWNU 395

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0.44 UTI
0.34
CN
0.61
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 6.3 [arcmin]
  • CN 0.34 Poorly populated
  • Cdens 0.61 Moderately dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 395 is a poorly populated, moderately dense object of high C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is poorly studied in the literature.
Relatively close Moderate 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 – 229.232 -53.687 0.549 -0.741 -1.426 –
Hunt & Reffert 2024 229.237 -53.677 0.541 -0.755 -1.415 –
Cavallo et al. 2024 229.243 -53.679 0.543 – – –
Hunt & Reffert 2023 229.237 -53.677 0.541 -0.755 -1.415 –
He et al. 2022 229.234 -53.682 0.54 -0.76 -1.4 –

💡 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 – – – – – 227* – –
Cavallo et al. 2024 1.77 1.48 – 81 0.340 – – –
Hunt & Reffert 2023 1.72 1.15 0.44 125 – – – –
He et al. 2022 1.95 1.14 – 316 0.537 – – –

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

Visualization

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