HSC 2526

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0.40 UTI
0.0
CN
1.0
Cdens
1.0
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 1.6 [arcmin]
  • CN 0.0 Sparse
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 2526 is a sparse, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by very high extinction. It is catalogued as a massive, 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 Very high extinction Massive Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Silver sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 190.349 -62.184 0.267 -6.826 -0.426 -34.31
Hunt & Reffert 2024 190.366 -62.184 0.289 -6.836 -0.426 -34.456
Cavallo et al. 2024 190.347 -62.19 0.284 – – –
Hunt & Reffert 2023 190.366 -62.184 0.289 -6.836 -0.426 -34.456

💡 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 – – – – – 1063* – –
Cavallo et al. 2024 3.44 5.18 – 245 0.130 – – –
Hunt & Reffert 2023 3.22 5.40 2.64 252 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3902 100.0 190.35 -62.18 0.3 -6.83 -0.43 -34.31 0.17

💡 Note: The % column shows the percentage of members that HSC 2526 shares with each listed object.

Visualization

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