CWNU 1179

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0.24 UTI
0.25
CN
0.22
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 72.0 [arcmin]
  • CN 0.25 Poorly populated
  • Cdens 0.22 Very loose
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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CWNU 1179 is a poorly populated, very loose object of high C3 quality. Its parallax locates it at a very close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is rarely studied in the literature.

âš ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Very close Low extinction Near-solar metallicity Young

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as a moving group.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 120.675 -57.772 4.404 -14.826 7.498 8.621
Cavallo et al. 2024 120.036 -56.895 4.265 – – –
Hunt & Reffert 2023 120.392 -57.9 4.272 -14.569 7.559 11.821
He et al. 2022 120.426 -58.16 4.436 -14.796 8.015 –

💡 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
Cavallo et al. 2024 0.23 0.83 – 19 -0.380 – – –
Hunt & Reffert 2023 0.24 0.92 0.71 45 – – – –
He et al. 2022 – 0.30 – 56 – – – –

Visualization

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