HSC 2332

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0.31 UTI
0.55
CN
0.25
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 4.3 [arcmin]
  • CN 0.55 Moderately populated
  • Cdens 0.25 Loose
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 2332 is a moderately populated, loose object of high C3 quality. Its parallax locates it at a large* distance, near the mid-plane, affected by high extinction. It is catalogued as a massive, near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.

(*): The parallax distance estimate (~5.46 kpc) differs significantly from the median photometric distance (~4.13 kpc).

Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.

Distant High extinction Massive Near-solar metallicity Young

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 – 155.597 -58.119 0.183 -5.546 3.17 66.673
Hunt & Reffert 2024 155.59 -58.119 0.189 -5.553 3.17 60.585
Cavallo et al. 2024 155.589 -58.135 0.189 – – –
Hunt & Reffert 2023 155.59 -58.119 0.189 -5.553 3.17 60.585

💡 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 – – – – – 1108* – –
Cavallo et al. 2024 3.61 3.15 – 66 0.130 – – –
Hunt & Reffert 2023 4.65 3.49 2.90 19 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3537 79.7 155.61 -58.12 0.19 -5.55 3.17 66.67 0.03

💡 Note: The % column shows the percentage of members that HSC 2332 shares with each listed object.

Visualization

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