HSC 2002

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0.35 UTI
0.0
CN
1.0
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 1.5 [arcmin]
  • CN 0.0 Sparse
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 2002 is a sparse, very dense object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by low 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 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 – 122.142 -30.805 0.223 -1.727 3.451 –
Hunt & Reffert 2024 122.146 -30.815 0.214 -1.728 3.449 –
Cavallo et al. 2024 122.129 -30.801 0.213 – – –
Hunt & Reffert 2023 122.146 -30.815 0.214 -1.728 3.449 –

💡 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 – – – – – 140* – –
Cavallo et al. 2024 4.19 0.89 – 105 0.230 – – –
Hunt & Reffert 2023 4.17 0.87 1.12 501 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3056 92.0 122.15 -30.8 0.22 -1.73 3.45 – 0.05

💡 Note: The % column shows the percentage of members that HSC 2002 shares with each listed object.

Visualization

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