HSC 1081

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0.17 UTI
0.0
CN
0.22
Cdens
0.62
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 3.9 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.22 Very loose
  • CC3 0.62 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 1081 is a sparse, very loose object of intermediate 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 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.

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 – 32.356 58.719 0.251 -1.216 0.111 -63.176
Hunt & Reffert 2024 32.324 58.717 0.247 -1.222 0.123 -29.69
Cavallo et al. 2024 32.376 58.704 0.247 – – –
Hunt & Reffert 2023 32.324 58.717 0.247 -1.222 0.123 -29.69

💡 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 – – – – – 162* – –
Cavallo et al. 2024 3.47 1.88 – 224 -0.320 – – –
Hunt & Reffert 2023 3.62 1.05 1.79 643 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3946 76.0 32.36 58.7 0.25 -1.22 0.11 -81.57 0.04

💡 Note: The % column shows the percentage of members that HSC 1081 shares with each listed object.

Visualization

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