HSC 2393

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0.33 UTI
0.0
CN
0.66
Cdens
1.0
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad) 3.3 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.66 Moderately dense
  • CC3 1.0 Very high quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 2393 is a sparse, moderately dense object of very high C3 quality. Its parallax locates it at a very large* distance, near the mid-plane, affected by high extinction. It is catalogued as a massive, metal-rich, intermediate-age cluster, but with a large variance across recent sources for the age parameter (see Parameters). It was recently reported in the literature.

(*): The parallax distance estimate (~10.05 kpc) differs significantly from the median photometric distance (~5.93 kpc).

Cavallo et al. (2024)
Silver 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– 165.086 -59.993 0.1 -5.516 2.483 36.872
Hunt & Reffert 2024 165.086 -59.994 0.102 -5.528 2.487 42.419
Cavallo et al. 2024 165.078 -59.992 0.099 – – –
Hunt & Reffert 2023 165.086 -59.994 0.102 -5.528 2.487 42.419

💡 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– 5.935 3.215 1.79 118 0.540 2361 – –
Hunt & Reffert 2024 – – – – – 2361(1) – –
Cavallo et al. 2024 2.94 2.61 – 229 0.540 – – –
Hunt & Reffert 2023 8.93 3.82 1.79 8 – – – –

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

Visualization

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