HSC 194

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0.35 UTI
0.25
CN
1.0
Cdens
0.5
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad) 5.8 [N/pc2]
  • CN 0.25 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.5 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 194 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.

Palma et al. (2025)
Classified as optical pair P450, along with UBC_97.

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 99999– 275.707 -15.001 0.73 -0.821 -3.338 -27.976
Hunt & Reffert 2024 275.735 -15.027 0.728 -0.79 -3.314 -26.279
Cavallo et al. 2024 275.712 -14.936 0.728 – – –
Hunt & Reffert 2023 275.735 -15.027 0.728 -0.79 -3.314 -26.279

💡 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– 1.195 1.15 0.82 612 0.020 105 – –
Hunt & Reffert 2024 – – – – – 105(1) – –
Cavallo et al. 2024 1.06 1.07 – 759 0.020 – – –
Hunt & Reffert 2023 1.33 1.23 0.82 465 – – – –

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

Visualization

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