HSC 1178

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0.09 UTI
0.0
CN
0.22
Cdens
0.25
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 6.3 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.22 Very loose
  • CC3 0.25 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 1178 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high 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 High extinction Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Silver sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 55.704 53.49 0.412 1.726 -1.859 -0.96
Hunt & Reffert 2024 55.59 53.503 0.414 1.732 -1.797 -0.979
Cavallo et al. 2024 55.667 53.488 0.411 – – –
Hunt & Reffert 2023 55.59 53.503 0.414 1.732 -1.797 -0.979

💡 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 – – – – – 308* – –
Cavallo et al. 2024 2.82 5.17 – 123 -0.100 – – –
Hunt & Reffert 2023 2.17 4.57 1.91 718 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3398 92.0 55.77 53.47 0.42 1.72 -1.83 -9.47 0.12

💡 Note: The % column shows the percentage of members that HSC 1178 shares with each listed object.

Visualization

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