HSC 1789

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0.32 UTI
0.0
CN
0.59
Cdens
0.5
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 1.8 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.59 Moderately dense
  • CC3 0.5 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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HSC 1789 is a sparse, moderately dense object of intermediate C3 quality. Its parallax locates it at a large* distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It was recently reported in the literature.

(*): The parallax distance estimate (~5.08 kpc) differs significantly from the median photometric distance (~3.71 kpc).

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

Distant Moderate extinction Near-solar metallicity 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 – 110.085 -12.137 0.197 -0.946 0.636 111.348
Hu & Soubiran 2025 110.073 -12.11 – – – –
Hunt & Reffert 2024 110.082 -12.129 0.194 -0.911 0.659 99.163
Cavallo et al. 2024 110.073 -12.11 0.193 – – –
Hunt & Reffert 2023 110.082 -12.129 0.194 -0.911 0.659 99.163

💡 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
Hu & Soubiran 2025 – – – – -0.290* – – –
Hunt & Reffert 2024 – – – – – 251* – –
Cavallo et al. 2024 3.08 2.14 – 617 -0.620 – – –
Hunt & Reffert 2023 4.34 1.40 1.94 538 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3156 80.0 110.09 -12.13 0.2 -0.96 0.64 103.81 0.07

💡 Note: The % column shows the percentage of members that HSC 1789 shares with each listed object.

Visualization

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