HSC 1118

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0.21 UTI
0.27
CN
0.54
Cdens
0.25
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 10.1 [arcmin]
  • CN 0.27 Poorly populated
  • Cdens 0.54 Moderately dense
  • CC3 0.25 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 1118 is a poorly populated, moderately dense object of low C3 quality. Its parallax locates it at a relatively close distance, near 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.

âš ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

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 – 41.737 57.286 0.932 2.749 -1.251 -26.659
Hunt & Reffert 2024 41.553 57.266 0.914 2.762 -1.258 -26.731
Cavallo et al. 2024 41.643 57.268 0.918 – – –
Hunt & Reffert 2023 41.553 57.266 0.914 2.762 -1.258 -26.731

💡 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
Hunt & Reffert 2024 – – – – – 82* – –
Cavallo et al. 2024 1.11 2.05 – 372 0.040 – – –
Hunt & Reffert 2023 1.02 1.74 0.58 398 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 4189 81.5 41.79 57.29 0.94 2.74 -1.23 -34.64 0.02

💡 Note: The % column shows the percentage of members that HSC 1118 shares with each listed object.

Visualization

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