HSC 591

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0.19 UTI
0.27
CN
0.44
Cdens
0.25
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 1.7 [arcmin]
  • CN 0.27 Poorly populated
  • Cdens 0.44 Loose
  • CC3 0.25 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 591 is a poorly populated, loose object of low C3 quality. Its parallax locates it at a large* distance, above the mid-plane, affected by high extinction. It is catalogued as a metal-rich, intermediate-age cluster (see Parameters). It was recently reported in the literature.

(*): The parallax distance estimate (~7.06 kpc) differs significantly from the median photometric distance (~5.12 kpc).

âš ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Very distant High extinction Metal-rich Intermediate age

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 – 302.74 38.256 0.142 -2.509 -4.84 -31.235
Hunt & Reffert 2024 302.745 38.252 0.144 -2.513 -4.816 -31.683
Cavallo et al. 2024 302.749 38.252 0.146 – – –
Hunt & Reffert 2023 302.745 38.252 0.144 -2.513 -4.816 -31.683

💡 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 – – – – – 752* – –
Cavallo et al. 2024 4.02 2.64 – 295 0.530 – – –
Hunt & Reffert 2023 6.21 3.43 2.24 112 – – – –

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Visualization

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