HSC 832

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0.43 UTI
0.5
CN
1.0
Cdens
0.62
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 1.7 [arcmin]
  • CN 0.5 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 0.62 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 832 is a moderately populated, very dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, young 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 High extinction Near-solar metallicity Young

Cavallo et al. (2024)
Bronze sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 338.947 60.006 0.34 -2.73 -1.71 -74.254
Hunt & Reffert 2024 338.947 60.007 0.36 -2.738 -1.705 -60.247
Cavallo et al. 2024 338.953 59.989 0.352 – – –
Hunt & Reffert 2023 338.947 60.007 0.36 -2.738 -1.705 -60.247

💡 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 – – – – – 497* – –
Cavallo et al. 2024 5.04 4.38 – 19 0.230 – – –
Hunt & Reffert 2023 2.69 4.40 2.96 30 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3334 82.4 338.94 60.01 0.34 -2.72 -1.71 -65.49 0.02

💡 Note: The % column shows the percentage of members that HSC 832 shares with each listed object.

Visualization

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