HSC 2520

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0.40 UTI
0.5
CN
0.76
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad) 3.8 [N/pc2]
  • CN 0.5 Moderately populated
  • Cdens 0.76 Dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 2520 is a moderately populated, dense object of 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, young cluster (see Parameters). It was recently reported in the literature.

(*): The parallax distance estimate (~4.61 kpc) differs significantly from the median photometric distance (~3.44 kpc).

Cavallo et al. (2024)
Bronze 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– 188.599 -62.268 0.217 -6.875 -0.074 -32.892
Hunt & Reffert 2024 188.576 -62.258 0.237 -6.812 -0.112 -32.835
Cavallo et al. 2024 189.11 -62.274 0.237 – – –
Hunt & Reffert 2023 188.576 -62.258 0.237 -6.812 -0.112 -32.835

💡 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– 3.445 5.315 3.21 24 -0.210 1317 – –
Hunt & Reffert 2024 – – – – – 1317(1) – –
Cavallo et al. 2024 3.16 5.25 – 30 -0.210 – – –
Hunt & Reffert 2023 3.73 5.38 3.21 18 – – – –

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

Visualization

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