HSC 2552

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0.34 UTI
0.42
CN
0.55
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad) 2.7 [N/pc2]
  • CN 0.42 Poorly populated
  • Cdens 0.55 Moderately dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 2552 is a poorly populated, moderately dense object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It was recently reported in the literature.

Palma et al. (2025)
Part of multiple system G59, along with CWNU_277, CWNU_2692, NGC_4755, Ruprecht_105 and CWNU_2664.

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 99999– 195.094 -60.604 0.46 -4.306 -1.242 –
Hunt & Reffert 2024 195.087 -60.619 0.464 -4.325 -1.243 –
Cavallo et al. 2024 195.07 -60.6 0.464 – – –
Hunt & Reffert 2023 195.087 -60.619 0.464 -4.325 -1.243 –

💡 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] Bfrac BSS
UCC 99999– 2.04 1.11 1.18 16 -0.170 199 – –
Hunt & Reffert 2024 – – – – – 199(1) – –
Cavallo et al. 2024 2.03 1.15 – 9 -0.170 – – –
Hunt & Reffert 2023 2.05 1.07 1.18 22 – – – –

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Visualization

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