HSC 2460

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0.28 UTI
0.27
CN
0.38
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 6.9 [arcmin]
  • CN 0.27 Poorly populated
  • Cdens 0.38 Loose
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 2460 is a poorly populated, loose object of high C3 quality. Its parallax locates it at a relatively close distance, above 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.
Relatively close 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 – 178.749 -58.732 0.535 -7.416 0.01 -42.895
Hunt & Reffert 2024 178.814 -58.739 0.534 -7.411 -0.009 -43.025
Cavallo et al. 2024 178.691 -58.755 0.535 – – –
Hunt & Reffert 2023 178.814 -58.739 0.534 -7.411 -0.009 -43.025

💡 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 – – – – – 206* – –
Cavallo et al. 2024 1.68 1.37 – 155 -0.150 – – –
Hunt & Reffert 2023 1.75 0.98 1.81 99 – – – –

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

Visualization

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