HSC 595

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0.52 UTI
0.59
CN
1.0
Cdens
1.0
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 1.6 [arcmin]
  • CN 0.59 Moderately 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 595 is a moderately 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, metal-rich, 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.

Relatively close Very high extinction Massive Metal-rich Intermediate age

Cavallo et al. (2024)
Gold sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 306.592 36.447 0.337 -1.827 -2.796 -10.069
Hunt & Reffert 2024 306.593 36.449 0.342 -1.844 -2.822 -10.074
Cavallo et al. 2024 306.594 36.452 0.335 – – –
Hunt & Reffert 2023 306.593 36.449 0.342 -1.844 -2.822 -10.074

💡 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 – – – – – 1257* – –
Cavallo et al. 2024 2.61 5.04 – 380 0.540 – – –
Hunt & Reffert 2023 2.57 5.21 2.58 229 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 2985 100.0 306.59 36.45 0.34 -1.8 -2.8 -10.07 0.18

💡 Note: The % column shows the percentage of members that HSC 595 shares with each listed object.

Visualization

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