HSC 2184

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0.30 UTI
0.26
CN
0.37
Cdens
0.38
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 1.9 [N/pc2]
  • CN 0.26 Poorly populated
  • Cdens 0.37 Loose
  • CC3 0.38 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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HSC 2184 is a poorly populated, loose object of low 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 (see Parameters). It was recently reported in the literature.

(*): The parallax distance estimate (~6.42 kpc) differs significantly from the median photometric distance (~4.74 kpc).

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

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 99999– 140.169 -45.995 0.156 -4.534 3.41 –
Hu & Soubiran 2025 140.182 -45.988 – – – –
Hunt & Reffert 2024 140.162 -45.998 0.161 -4.511 3.399 –
Cavallo et al. 2024 140.182 -45.988 0.17 – – –
Hunt & Reffert 2023 140.162 -45.998 0.161 -4.511 3.399 –

💡 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] Bfrac BSS
UCC 99999– 4.735 2.505 1.67 804 -0.020 483 – –
Hu & Soubiran 2025 – – – – -0.100(5) – – –
Hunt & Reffert 2024 – – – – – 483(1) – –
Cavallo et al. 2024 4.23 2.48 – 813 0.060 – – –
Hunt & Reffert 2023 5.24 2.53 1.67 794 – – – –

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3209 88.5 140.17 -45.99 0.16 -4.54 3.41 – 0.01

💡 Note: The % column shows the percentage of members that HSC 2184 shares with each listed object.

Visualization

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