HSC 2088

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0.06 UTI
0.28
CN
0.16
Cdens
0.5
CC3
0.0
Clit
0.32
Cdup
Radius (P>50% members) 4.5 [arcmin]
  • CN 0.28 Poorly populated
  • Cdens 0.16 Very loose
  • CC3 0.5 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 0.32 Possibly duplicate

Overview

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HSC 2088 is a poorly populated, very loose 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.

âš ī¸ Warning: This is possibly a duplicate object, which shares a significant percentage of members with at least one previously 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 – 123.014 -44.126 0.221 -2.524 4.263 –
Hunt & Reffert 2024 123.021 -44.121 0.222 -2.535 4.315 –
Cavallo et al. 2024 123.021 -44.119 0.223 – – –
Hunt & Reffert 2023 123.021 -44.121 0.222 -2.535 4.315 –

💡 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 – – – – – 275* – –
Cavallo et al. 2024 4.23 2.51 – 145 0.030 – – –
Hunt & Reffert 2023 4.05 2.18 1.77 107 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 2814 67.9 123.09 -44.2 0.23 -2.52 4.24 86.0 0.14

💡 Note: The % column shows the percentage of members that HSC 2088 shares with each listed object.

Visualization

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