HSC 2528

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0.11 UTI
0.0
CN
1.0
Cdens
0.75
CC3
0.0
Clit
0.32
Cdup
Radius (P>50% members) 3.7 [arcmin]
  • CN 0.0 Sparse
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 0.32 Possibly duplicate

Overview

â„šī¸
HSC 2528 is a sparse, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, above 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.

Relatively close 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 – 190.871 -60.755 0.679 -6.377 0.048 -14.256
Hunt & Reffert 2024 190.86 -60.748 0.674 -6.369 0.043 -14.238
Cavallo et al. 2024 190.872 -60.748 0.678 – – –
Hunt & Reffert 2023 190.86 -60.748 0.674 -6.369 0.043 -14.238

💡 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 – – – – – 125* – –
Cavallo et al. 2024 1.56 1.36 – 174 -0.050 – – –
Hunt & Reffert 2023 1.39 0.90 0.45 461 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 14186 68.0 190.93 -60.76 0.68 -6.4 0.0 -1.35 0.19

💡 Note: The % column shows the percentage of members that HSC 2528 shares with each listed object.

Visualization

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