HSC 1788

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0.07 UTI
0.0
CN
0.08
Cdens
0.25
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 6.7 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.08 Very loose
  • CC3 0.25 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 1788 is a sparse, very loose 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.

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 – 109.133 -12.507 0.29 -2.069 2.152 –
Hunt & Reffert 2024 109.14 -12.559 0.283 -2.063 2.164 –
Cavallo et al. 2024 109.16 -12.507 0.286 – – –
Hunt & Reffert 2023 109.14 -12.559 0.283 -2.063 2.164 –

💡 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 – – – – – 149* – –
Cavallo et al. 2024 2.82 1.31 – 148 0.130 – – –
Hunt & Reffert 2023 3.02 1.41 0.47 93 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3811 76.0 109.13 -12.44 0.29 -2.09 2.15 82.3 0.04

💡 Note: The % column shows the percentage of members that HSC 1788 shares with each listed object.

Visualization

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