HSC 2416

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0.10 UTI
0.0
CN
0.11
Cdens
0.38
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 5.0 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.11 Very loose
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 2416 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a metal-rich, intermediate-age 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 Moderate extinction Metal-rich 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 – 167.823 -62.757 0.243 -5.155 1.17 -10.178
Hunt & Reffert 2024 167.701 -62.737 0.239 -5.125 1.193 -8.103
Cavallo et al. 2024 167.933 -62.837 0.24 – – –
Hunt & Reffert 2023 167.701 -62.737 0.239 -5.125 1.193 -8.103

💡 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 – – – – – 122* – –
Cavallo et al. 2024 3.89 2.64 – 288 0.520 – – –
Hunt & Reffert 2023 3.65 2.88 2.30 115 – – – –

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

Visualization

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