HSC 2431

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0.43 UTI
0.42
CN
1.0
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 4.2 [arcmin]
  • CN 0.42 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 2431 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.
Relatively close Low 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 – 174.192 -57.645 0.495 -8.224 1.489 -20.988
Hunt & Reffert 2024 174.186 -57.613 0.499 -8.217 1.52 –
Cavallo et al. 2024 174.155 -57.641 0.499 – – –
Hunt & Reffert 2023 174.186 -57.613 0.499 -8.217 1.52 –

💡 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 – – – – – 180* – –
Cavallo et al. 2024 1.71 0.77 – 182 -0.300 – – –
Hunt & Reffert 2023 1.89 0.44 0.43 94 – – – –

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

Visualization

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