HSC 571

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0.48 UTI
0.42
CN
1.0
Cdens
1.0
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad) 10.4 [N/pc2]
  • CN 0.42 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 571 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 very high extinction. It is catalogued as a massive, near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age parameter (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.

Cavallo et al. (2024)
Wood 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– 304.176 34.43 0.217 -2.211 -4.561 -20.621
Hunt & Reffert 2024 304.17 34.433 0.218 -2.216 -4.565 -20.962
Cavallo et al. 2024 304.17 34.43 0.221 – – –
Hunt & Reffert 2023 304.17 34.433 0.218 -2.216 -4.565 -20.962

💡 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– 3.9 5.705 2.6 374 0.370 2700 – –
Hunt & Reffert 2024 – – – – – 2700(1) – –
Cavallo et al. 2024 3.98 5.65 – 95 0.370 – – –
Hunt & Reffert 2023 3.82 5.76 2.60 652 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3271 100.0 304.18 34.43 0.22 -2.22 -4.57 -20.62 0.26

💡 Note: The % column shows the percentage of members that HSC 571 shares with each listed object.

Visualization

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