CWNU 364

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0.54 UTI
0.33
CN
1.0
Cdens
0.75
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members) 7.5 [arcmin]
  • CN 0.33 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.31 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 364 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a close distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It is poorly studied in the literature.
Close Low extinction Near-solar metallicity Very 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 – 55.005 43.228 1.032 -1.278 -3.635 -17.212
Zhang et al. 2024 55.009 43.204 – – – –
Hunt & Reffert 2024 55.009 43.204 1.017 -1.264 -3.643 -20.997
Cavallo et al. 2024 54.94 43.276 1.024 – – –
Hunt & Reffert 2023 55.009 43.204 1.017 -1.264 -3.643 -20.997
He et al. 2022 54.966 43.246 1.02 -1.27 -3.63 –

💡 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 – – – – -0.114* – – –
Hunt & Reffert 2024 – – – – – 135* – –
Cavallo et al. 2024 1.12 1.35 – 5 -0.270 – – –
Hunt & Reffert 2023 0.92 0.93 0.72 12 – – – –
He et al. 2022 0.71 0.90 – 13 -0.930 – – –

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

Visualization

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