HSC 571

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0.48 UTI
0.42
CN
1.0
Cdens
1.0
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 1.5 [arcmin]
  • 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 (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.

Distant Very high extinction Massive Near-solar metallicity Intermediate age

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 – 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] Bfr BSS
Hunt & Reffert 2024 – – – – – 2700* – –
Cavallo et al. 2024 3.98 5.65 – 95 0.370 – – –
Hunt & Reffert 2023 3.82 5.76 2.60 652 – – – –

(*): Indicates that this parameter is assigned more than one value 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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