HSC 2331

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0.40 UTI
0.27
CN
1.0
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 1.0 [arcmin]
  • CN 0.27 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 2331 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.
Relatively close Moderate extinction Near-solar metallicity Young

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 – 156.544 -57.175 0.357 -7.269 3.641 –
Hunt & Reffert 2024 156.543 -57.175 0.36 -7.277 3.622 –
Cavallo et al. 2024 156.568 -57.178 0.358 – – –
Hunt & Reffert 2023 156.543 -57.175 0.36 -7.277 3.622 –

💡 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 – – – – – 229* – –
Cavallo et al. 2024 2.86 2.18 – 78 0.140 – – –
Hunt & Reffert 2023 2.53 1.80 1.72 36 – – – –

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

Visualization

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