CWNU 495

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0.50 UTI
0.57
CN
0.7
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 3.5 [N/pc2]
  • CN 0.57 Moderately populated
  • Cdens 0.7 Moderately dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
CWNU 495 is a moderately populated, moderately dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a metal-rich, young cluster, but with a large variance across recent sources for the age parameter (see Parameters). It is poorly studied in the literature.

Palma et al. (2025)
Classified as tidal capture (resonant trapping pair) P208, along with UBC_1120.

Cavallo et al. (2024)
Silver sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 317.514 45.027 0.481 -2.608 -3.892 -27.084
Hunt & Reffert 2024 317.52 45.039 0.477 -2.58 -3.893 -32.976
Cavallo et al. 2024 317.477 45.033 0.478 – – –
Hunt & Reffert 2023 317.52 45.039 0.477 -2.58 -3.893 -32.976
He et al. 2022 317.495 45.029 0.48 -2.62 -3.9 –

💡 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] Bfrac BSS
UCC 99999– 2.5 2.15 2.29 60 0.540 620 – –
Hunt & Reffert 2024 – – – – – 620(1) – –
Cavallo et al. 2024 2.50 2.15 – 60 0.400 – – –
Hunt & Reffert 2023 1.97 1.52 2.29 114 – – – –
He et al. 2022 3.55 2.58 – 5 0.680 – – –

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Visualization

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