HSC 2354

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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) 1.4 [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 2354 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, below 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.

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

Distant 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 – 158.752 -59.635 0.21 -5.501 2.401 16.279
Hunt & Reffert 2024 158.759 -59.631 0.209 -5.495 2.401 16.29
Cavallo et al. 2024 158.741 -59.639 0.208 – – –
Hunt & Reffert 2023 158.759 -59.631 0.209 -5.495 2.401 16.29

💡 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 – – – – – 700* – –
Cavallo et al. 2024 3.16 2.73 – 229 -0.480 – – –
Hunt & Reffert 2023 4.30 2.77 2.14 92 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3684 100.0 158.74 -59.64 0.22 -5.48 2.38 16.28 0.17

💡 Note: The % column shows the percentage of members that HSC 2354 shares with each listed object.

Visualization

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