CWNU 96

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0.43 UTI
0.52
CN
0.26
Cdens
0.75
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members) 23.8 [arcmin]
  • CN 0.52 Moderately populated
  • Cdens 0.26 Loose
  • CC3 0.75 High quality
  • Clit 0.31 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 96 is a moderately populated, loose object of high C3 quality. Its parallax locates it at a close distance, near 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.
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 – 312.541 38.31 1.075 -3.315 -4.236 -1.339
Zhang et al. 2024 312.487 38.32 – – – –
Hunt & Reffert 2024 312.487 38.32 1.057 -3.353 -4.23 -0.841
Cavallo et al. 2024 312.634 38.318 1.066 – – –
Hunt & Reffert 2023 312.487 38.32 1.057 -3.353 -4.23 -0.841
He et al. 2022 312.72 38.361 1.08 -3.3 -4.22 –

💡 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
Zhang et al. 2024 – – – – -0.124* – – –
Hunt & Reffert 2024 – – – – – 63* – –
Cavallo et al. 2024 0.98 0.97 – 24 -0.250 – – –
Hunt & Reffert 2023 0.89 0.56 1.05 39 – – – –
He et al. 2022 0.93 0.96 – 40 -0.082 – – –

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

Visualization

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