HSC 2139

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0.30 UTI
0.52
CN
0.23
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad) 1.1 [N/pc2]
  • CN 0.52 Moderately populated
  • Cdens 0.23 Very loose
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 2139 is a moderately populated, very loose object of high C3 quality. Its parallax locates it at a very close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, very young cluster, but with a large variance across recent sources for the absorption parameter (see Parameters). It was recently reported in the literature.

Liu et al. (2025)
Classified as primordial binary cluster 217 along with HSC_2068.

Palma et al. (2025)
Part of multiple system G138, along with HSC_2068, HSC_2156 and Platais_9.

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as a moving group.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 127.485 -49.771 5.285 -7.944 7.873 20.789
Cavallo et al. 2024 127.318 -49.919 5.294 – – –
Hunt & Reffert 2023 128.381 -47.518 5.308 -7.866 7.974 21.108

💡 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– 0.19 0.12 0.33 17 -0.140 – – –
Liu et al. 2025 0.18 0.04 – 38 – – – –
Cavallo et al. 2024 0.19 0.54 – 17 -0.140 – – –
Hunt & Reffert 2023 0.19 0.12 0.33 12 – – – –

Visualization

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