HSC 1786

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0.18 UTI
0.34
CN
0.17
Cdens
0.38
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 8.0 [arcmin]
  • CN 0.34 Poorly populated
  • Cdens 0.17 Very loose
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 1786 is a poorly populated, very loose object of low C3 quality. Its parallax locates it at a moderate distance, above 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 significant 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 – 110.869 -11.563 0.365 -2.225 2.202 –
Hunt & Reffert 2024 110.863 -11.521 0.339 -2.196 2.211 70.501
Cavallo et al. 2024 110.936 -11.674 0.34 – – –
Hunt & Reffert 2023 110.863 -11.521 0.339 -2.196 2.211 70.501

💡 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 – – – – – 200* – –
Cavallo et al. 2024 2.82 1.32 – 51 0.140 – – –
Hunt & Reffert 2023 2.55 1.00 1.83 189 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3832 55.9 110.88 -11.62 0.36 -2.22 2.19 – 0.03

💡 Note: The % column shows the percentage of members that HSC 1786 shares with each listed object.

Visualization

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