HSC 1832

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0.20 UTI
0.0
CN
0.65
Cdens
0.38
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 2.8 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.65 Moderately dense
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 1832 is a sparse, moderately dense object of 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.

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.

Distant 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 – 110.313 -17.185 0.306 -2.312 2.814 –
Hunt & Reffert 2024 110.31 -17.179 0.31 -2.32 2.813 –
Cavallo et al. 2024 110.321 -17.189 0.31 – – –
Hunt & Reffert 2023 110.31 -17.179 0.31 -2.32 2.813 –

💡 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 – – – – – 193* – –
Cavallo et al. 2024 3.13 2.53 – 87 0.080 – – –
Hunt & Reffert 2023 3.12 2.40 1.55 201 – – – –

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

Visualization

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