HSC 2592

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0.37 UTI
0.33
CN
1.0
Cdens
0.5
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 1.5 [arcmin]
  • CN 0.33 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.5 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 2592 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.

Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.

Distant High extinction Near-solar metallicity Intermediate age

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 – 202.473 -62.497 0.242 -6.02 -1.74 -53.743
Hunt & Reffert 2024 202.447 -62.495 0.233 -6.016 -1.745 -43.16
Cavallo et al. 2024 202.492 -62.49 0.234 – – –
Hunt & Reffert 2023 202.447 -62.495 0.233 -6.016 -1.745 -43.16

💡 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 – – – – – 472* – –
Cavallo et al. 2024 3.15 4.23 – 331 -0.390 – – –
Hunt & Reffert 2023 3.81 4.11 2.57 54 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 4114 100.0 202.5 -62.49 0.24 -6.02 -1.74 -53.16 0.27

💡 Note: The % column shows the percentage of members that HSC 2592 shares with each listed object.

Visualization

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