HSC 2178

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0.12 UTI
0.0
CN
0.33
Cdens
0.25
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 4.2 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.33 Loose
  • CC3 0.25 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 2178 is a sparse, loose object of low C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by high extinction. It is catalogued as a metal-rich, young cluster (see Parameters). It was recently reported in the literature.

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 High extinction Metal-rich Young

Cavallo et al. (2024)
Bronze sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 137.637 -46.986 0.328 -3.96 3.913 83.805
Hunt & Reffert 2024 137.606 -46.982 0.342 -3.991 3.927 169.572
Cavallo et al. 2024 137.672 -46.982 0.338 – – –
Hunt & Reffert 2023 137.606 -46.982 0.342 -3.991 3.927 169.572

💡 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 – – – – – 374* – –
Cavallo et al. 2024 3.37 4.69 – 42 0.520 – – –
Hunt & Reffert 2023 2.70 5.16 2.64 50 – – – –

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

Visualization

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