HSC 1937

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0.38 UTI
0.0
CN
0.9
Cdens
0.5
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 1.5 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.9 Very dense
  • CC3 0.5 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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HSC 1937 is a sparse, very dense object of intermediate C3 quality. Its parallax locates it at a large distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, old 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 Low extinction Near-solar metallicity Old

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 – 110.888 -28.605 0.193 -1.544 2.16 51.868
Hu & Soubiran 2025 110.892 -28.61 – – – –
Hunt & Reffert 2024 110.882 -28.603 0.193 -1.535 2.16 46.635
Cavallo et al. 2024 110.892 -28.61 0.197 – – –
Hunt & Reffert 2023 110.882 -28.603 0.193 -1.535 2.16 46.635

💡 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 – – – – -0.310* – – –
Hunt & Reffert 2024 – – – – – 246* – –
Cavallo et al. 2024 4.07 1.26 – 1148 -0.440 – – –
Hunt & Reffert 2023 4.84 0.63 1.22 1607 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3036 100.0 110.88 -28.61 0.19 -1.55 2.16 51.87 0.04

💡 Note: The % column shows the percentage of members that HSC 1937 shares with each listed object.

Visualization

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