HSC 1920

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0.03 UTI
0.0
CN
0.14
Cdens
0.5
CC3
0.0
Clit
0.24
Cdup
Radius (P>50% members) 27.5 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.14 Very loose
  • CC3 0.5 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 0.24 Likely duplicate

Overview

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HSC 1920 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a close distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It was recently reported in the literature.

âš ī¸ Warning: This is likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

Close Low extinction Near-solar metallicity Very young

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 – 99.534 -31.67 1.509 -2.971 4.448 36.878
Cavallo et al. 2024 99.348 -31.725 1.499 – – –
Hunt & Reffert 2023 98.224 -32.058 1.498 -2.905 4.401 27.399

💡 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] Bfr BSS
Cavallo et al. 2024 0.74 0.54 – 10 -0.150 – – –
Hunt & Reffert 2023 0.63 0.19 0.80 17 – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 20 76.0 99.81 -31.61 1.51 -2.99 4.44 22.64 0.18

💡 Note: The % column shows the percentage of members that HSC 1920 shares with each listed object.

Visualization

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