HSC 2579

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0.50 UTI
0.48
CN
1.0
Cdens
1.0
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad) 5.1 [N/pc2]
  • CN 0.48 Poorly populated
  • 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 2579 is a poorly populated, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a metal-rich, young cluster, but with a large variance across recent sources for the age parameter (see Parameters). It was recently reported in the literature.

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 99999– 200.173 -62.843 0.266 -6.142 -1.41 43.585
Hunt & Reffert 2024 200.147 -62.846 0.265 -6.126 -1.396 62.757
Cavallo et al. 2024 200.179 -62.85 0.267 – – –
Hunt & Reffert 2023 200.147 -62.846 0.265 -6.126 -1.396 62.757

💡 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– 2.915 3.36 2.52 84 0.650 814 – –
Hunt & Reffert 2024 – – – – – 814(1) – –
Cavallo et al. 2024 2.36 3.05 – 158 0.650 – – –
Hunt & Reffert 2023 3.47 3.67 2.52 10 – – – –

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

Visualization

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