HSC 1831

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0.11 UTI
0.26
CN
0.18
Cdens
0.12
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 6.8 [arcmin]
  • CN 0.26 Poorly populated
  • Cdens 0.18 Very loose
  • CC3 0.12 Very low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 1831 is a poorly populated, very loose object of very low C3 quality. Its parallax locates it at a moderate distance, near 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.

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

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.

Relatively close Moderate extinction 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 – 111.696 -16.333 0.365 -3.029 3.575 89.989
Hunt & Reffert 2024 111.661 -16.433 0.347 -3.033 3.564 –
Cavallo et al. 2024 111.705 -16.317 0.338 – – –
Hunt & Reffert 2023 111.661 -16.433 0.347 -3.033 3.564 –

💡 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 – – – – – 115* – –
Cavallo et al. 2024 3.34 2.09 – 245 0.320 – – –
Hunt & Reffert 2023 2.51 1.87 1.56 144 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3752 88.5 111.7 -16.32 0.35 -3.06 3.59 58.33 0.05

💡 Note: The % column shows the percentage of members that HSC 1831 shares with each listed object.

Visualization

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