HSC 2523

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0.25 UTI
0.0
CN
1.0
Cdens
0.75
CC3
0.0
Clit
0.72
Cdup
Radius (P>50% members) 60.5 [arcmin]
  • CN 0.0 Sparse
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 0.72 Likely unique

Overview

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HSC 2523 is a sparse, very dense object of high C3 quality. Its parallax locates it at a very close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.

Note: This is likely a unique object, which shares a moderate percentage of members with at least one previously reported entry. See table with shared members information.

Very close Moderate extinction Near-solar metallicity Young

Cavallo et al. (2024)
Bronze sample.

Hunt & Reffert (2024)
Classified as a moving group.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 187.321 -72.919 9.841 -39.683 -10.808 12.789
Cavallo et al. 2024 186.982 -72.98 9.842 – – –
Hunt & Reffert 2023 187.535 -72.94 9.848 -39.79 -10.534 11.552

💡 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
Cavallo et al. 2024 0.11 1.68 – 35 -0.240 – – –
Hunt & Reffert 2023 0.10 1.15 0.95 7 – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
Feigelson 1 28.0 180.43 -76.37 9.74 -40.27 -6.17 13.74 0.7

💡 Note: The % column shows the percentage of members that HSC 2523 shares with each listed object.

Visualization

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