HSC 393

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0.37 UTI
0.35
CN
1.0
Cdens
0.5
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad) 13.5 [N/pc2]
  • CN 0.35 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 393 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by very high extinction. It is catalogued as a massive, metal-rich, young cluster, but with a large variance across recent sources for the age parameter (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– 289.769 11.1 0.433 -1.97 -4.456 17.471
Hunt & Reffert 2024 289.789 11.103 0.416 -1.993 -4.469 -33.574
Cavallo et al. 2024 289.758 11.093 0.422 – – –
Hunt & Reffert 2023 289.789 11.103 0.416 -1.993 -4.469 -33.574

💡 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– 2.655 5.28 2.78 57 0.630 1321 – –
Hunt & Reffert 2024 – – – – – 1321(1) – –
Cavallo et al. 2024 3.05 4.76 – 13 0.630 – – –
Hunt & Reffert 2023 2.26 5.80 2.78 101 – – – –

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

Visualization

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