HSC 2363

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0.09 UTI
0.78
CN
1.0
Cdens
1.0
CC3
0.0
Clit
0.16
Cdup
Radius (P>50% members) 2.1 [arcmin]
  • CN 0.78 Rich
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.0 Rarely studied
  • Cdup 0.16 Likely duplicate

Overview

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HSC 2363 is a rich, very dense object of very high C3 quality. Its parallax locates it at a large distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It was recently reported in the literature.

âš ī¸ Warning: This is likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

Very distant Moderate extinction Near-solar metallicity Intermediate age

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 – 158.811 -60.691 0.14 -4.861 2.544 37.722
Hu & Soubiran 2025 158.806 -60.681 – – – –
Cavallo et al. 2024 158.806 -60.681 0.14 – – –
Hunt & Reffert 2023 158.819 -60.694 0.143 -4.878 2.548 30.776

💡 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
Hu & Soubiran 2025 – – – – -0.460* – – –
Cavallo et al. 2024 4.88 1.85 – 1072 -0.150 – – –
Hunt & Reffert 2023 6.41 2.12 2.36 617 – – – –

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3141 92.7 158.82 -60.69 0.14 -4.85 2.55 29.28 0.09
Teutsch 105 83.7 158.81 -60.69 0.14 -4.86 2.55 37.72 0.55

💡 Note: The % column shows the percentage of members that HSC 2363 shares with each listed object.

Visualization

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