HSC 1064

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0.33 UTI
0.28
CN
1.0
Cdens
0.38
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 3.3 [arcmin]
  • CN 0.28 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 1064 is a poorly populated, very dense object of low C3 quality. Its parallax locates it at a moderate 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 – 32.303 65.015 0.487 1.934 -1.712 -2.434
Hunt & Reffert 2024 32.329 65.013 0.479 1.883 -1.719 -2.465
Cavallo et al. 2024 32.45 65.02 0.477 – – –
Hunt & Reffert 2023 32.329 65.013 0.479 1.883 -1.719 -2.465

💡 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 – – – – – 56* – –
Cavallo et al. 2024 1.80 2.28 – 316 0.160 – – –
Hunt & Reffert 2023 1.96 2.21 0.96 405 – – – –

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

Visualization

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