HSC 2290

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0.32 UTI
0.0
CN
0.58
Cdens
0.5
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 7.4 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.58 Moderately dense
  • CC3 0.5 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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HSC 2290 is a sparse, moderately dense object of intermediate C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It was recently reported in the literature.
Relatively close Low 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 – 147.454 -58.008 0.797 -6.42 3.486 9.198
Hu & Soubiran 2025 147.454 -58.047 – – – –
Hunt & Reffert 2024 147.549 -58.079 0.8 -6.431 3.535 6.316
Cavallo et al. 2024 147.454 -58.047 0.799 – – –
Hunt & Reffert 2023 147.549 -58.079 0.8 -6.431 3.535 6.316

💡 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
Hu & Soubiran 2025 – – – – -0.320* – – –
Hunt & Reffert 2024 – – – – – 59* – –
Cavallo et al. 2024 1.16 0.52 – 661 0.340 – – –
Hunt & Reffert 2023 1.21 0.38 1.02 270 – – – –

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

Visualization

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