HSC 2595

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0.45 UTI
0.52
CN
0.98
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 6.1 [arcmin]
  • CN 0.52 Moderately populated
  • Cdens 0.98 Very dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 2595 is a moderately populated, very dense 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, young cluster (see Parameters). It was recently reported in the literature.
Relatively close Moderate extinction Near-solar metallicity Young

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 – 202.747 -60.933 0.528 -4.848 -1.842 -4.327
Hunt & Reffert 2024 202.751 -60.938 0.527 -4.878 -1.871 –
Cavallo et al. 2024 202.743 -60.916 0.528 – – –
Hunt & Reffert 2023 202.751 -60.938 0.527 -4.878 -1.871 –

💡 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 – – – – – 218* – –
Cavallo et al. 2024 1.67 1.10 – 13 -0.090 – – –
Hunt & Reffert 2023 1.77 0.96 1.53 74 – – – –

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

Visualization

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