HSC 350

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0.32 UTI
0.33
CN
0.76
Cdens
0.5
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad) 3.8 [N/pc2]
  • CN 0.33 Poorly populated
  • Cdens 0.76 Dense
  • CC3 0.5 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 350 is a poorly populated, dense object of intermediate C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by very high extinction. It is catalogued as a metal-poor, intermediate-age cluster (see Parameters). It was recently reported in the literature.

Cavallo et al. (2024)
Bronze 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– 284.632 5.02 0.838 3.812 0.468 23.181
Hunt & Reffert 2024 284.584 5.046 0.842 3.769 0.47 24.983
Cavallo et al. 2024 284.63 5.003 0.842 – – –
Hunt & Reffert 2023 284.584 5.046 0.842 3.769 0.47 24.983

💡 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– 1.49 5.02 2.69 142 -0.660 276 – –
Hunt & Reffert 2024 – – – – – 276(1) – –
Cavallo et al. 2024 1.85 4.99 – 126 -0.660 – – –
Hunt & Reffert 2023 1.13 5.05 2.69 158 – – – –

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

Visualization

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