CWNU 1198

(OCSN 124)

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0.39 UTI
0.27
CN
0.91
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
C3 classification AB
Number of members (P>50%) 27
Radius (P>50% members) 18.9 [arcmin]
  • CN 0.27 Poorly populated
  • Cdens 0.91 Very dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique
đŸ“Ĩ Members 📊 Colab đŸ”Ŧ Bayestar19 🔍 CDS 🔍 Simbad 🔍 CDS (Îą, δ) 🔍 Simbad (Îą, δ)

Overview
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CWNU 1198 is a poorly populated, very dense 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 young cluster (see Parameters). It is rarely studied in the literature.
Close Low extinction Young

Data
🔍 Search references for CWNU 1198 in: SciX Simbad
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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 183.929 -70.569 2.258 -13.092 -1.795 7.91
Qin et al. 2023 183.89 -70.62 2.19 -13.23 -1.77 7.31
He et al. 2022 184.178 -70.608 2.279 -13.072 -1.888 –

💡 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
Qin et al. 2023 0.63 0.81 – 35 – – – –
He et al. 2022 – 0.75 – 40 – – – –

Visualization
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CWNU 1198 UCC
Galactocentric position diagram