HSC 1922

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0.17 UTI
0.29
CN
0.21
Cdens
0.38
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 19.2 [arcmin]
  • CN 0.29 Poorly populated
  • Cdens 0.21 Very loose
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 1922 is a poorly populated, very loose object of low C3 quality. Its parallax locates it at a close distance, below the mid-plane, affected by low extinction. It is catalogued as a low-mass, near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.

âš ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Close Low extinction Low mass 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 – 111.392 -26.776 1.059 -3.461 4.029 43.324
Hunt & Reffert 2024 111.397 -26.798 1.047 -3.409 3.975 39.696
Cavallo et al. 2024 111.385 -26.773 1.055 – – –
Hunt & Reffert 2023 111.397 -26.798 1.047 -3.409 3.975 39.696

💡 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
Hunt & Reffert 2024 – – – – – 48* – –
Cavallo et al. 2024 0.93 0.10 – 229 0.400 – – –
Hunt & Reffert 2023 0.91 0.08 0.37 188 – – – –

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

Visualization

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