HSC 1180

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0.16 UTI
0.0
CN
0.06
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 6.6 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.06 Very loose
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 1180 is a sparse, very loose object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a metal-rich, young 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.

Very distant Moderate extinction Metal-rich Young

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 – 64.169 58.079 0.22 -0.0 -0.101 -105.832
Hunt & Reffert 2024 64.205 58.057 0.225 -0.018 -0.092 -105.834
Cavallo et al. 2024 64.192 58.071 0.221 – – –
Hunt & Reffert 2023 64.205 58.057 0.225 -0.018 -0.092 -105.834

💡 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 – – – – – 288* – –
Cavallo et al. 2024 7.05 2.62 – 47 0.520 – – –
Hunt & Reffert 2023 4.01 2.37 1.67 66 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3809 92.0 64.19 58.08 0.22 -0.01 -0.1 -105.83 0.02

💡 Note: The % column shows the percentage of members that HSC 1180 shares with each listed object.

Visualization

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