CWNU 1173

(OCSN 184)

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0.55 UTI
0.26
CN
1.0
Cdens
1.0
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 13.5 [arcmin]
  • CN 0.26 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 1173 is a poorly populated, very dense object of very 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 poorly studied in the literature.
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 – 179.897 -70.2 2.277 -13.182 -0.801 7.351
Cavallo et al. 2024 178.989 -70.126 2.251 – – –
Hunt & Reffert 2023 179.922 -70.286 2.244 -13.031 -0.622 5.449
Qin et al. 2023 179.64 -70.33 2.25 -13.27 -0.51 4.38
He et al. 2022 179.942 -70.323 2.29 -13.198 -0.811 –

💡 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 0.46 0.91 – 23 0.230 – – –
Hunt & Reffert 2023 0.42 0.50 0.99 100 – – – –
Qin et al. 2023 0.61 0.78 – 35 – – – –
He et al. 2022 – 0.80 – 22 – – – –

Visualization

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