HSC 1117

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0.26 UTI
0.36
CN
0.11
Cdens
0.75
CC3
0.03
Clit
1.0
Cdup
Core radius and density 3.2 [pc], 0.5 [pc-2]
  • CN 0.36 Poorly populated
  • Cdens 0.11 Very loose
  • CC3 0.75 High quality
  • Clit 0.03 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 1117 is a poorly populated, very loose object of high C3 quality. Its parallax locates it at a large distance, well above 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 object shares a large percentage of members with a later reported entry. See table with shared members information.

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.15 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.15 (50th percentile).

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 50.097 65.067 0.161 -0.312 0.164 –
Hunt & Reffert 2024 50.107 65.055 0.155 -0.317 0.171 –
Cavallo et al. 2024 50.056 65.089 0.165 – – –
Hunt & Reffert 2023 50.107 65.055 0.155 -0.317 0.171 –

💡 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– 5.62 2.6 1.6 197 0.050 525 – –
Hunt & Reffert 2024 5.62 2.60 1.60 197 – 525(1) – –
Cavallo et al. 2024 4.76 2.85 – 58 0.050 – – –
Hunt & Reffert 2023 5.62 2.60 1.60 197 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3672 100.0 50.09 65.07 0.16 -0.31 0.16 -72.19 0.07

💡 Note: The % column shows the percentage of members that HSC 1117 shares with each listed object.

Visualization

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