HSC 893

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0.35 UTI
0.32
CN
1.0
Cdens
0.25
CC3
0.25
Clit
0.84
Cdup
Radius (P>50% members) 2.7 [arcmin]
  • CN 0.32 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.25 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 0.84 Very likely unique

Overview

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HSC 893 is a poorly populated, very dense object of low C3 quality. Its parallax locates it at a moderate distance, below 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.

Note: This is very likely a unique object, which shares a small percentage of members with at least one previously reported entry. See table with shared members information.

Relatively close 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 – 352.028 57.694 0.37 -1.539 -1.172 -3.592
Hu & Soubiran 2025 352.034 57.692 – – – –
Hunt & Reffert 2024 352.036 57.717 0.377 -1.556 -1.174 -3.451
Cavallo et al. 2024 352.034 57.692 0.376 – – –
Hunt & Reffert 2023 352.036 57.717 0.377 -1.556 -1.174 -3.451

💡 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 – – – – 0.090* – – –
Hunt & Reffert 2024 – – – – – 287* – –
Cavallo et al. 2024 2.59 2.33 – 501 0.070 – – –
Hunt & Reffert 2023 2.46 2.23 0.81 528 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 1640 15.6 352.69 57.81 0.42 -1.56 -1.11 – 0.06

💡 Note: The % column shows the percentage of members that HSC 893 shares with each listed object.

Visualization

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