HSC 1783

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0.19 UTI
0.37
CN
0.21
Cdens
0.38
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 5.7 [arcmin]
  • CN 0.37 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 1783 is a poorly populated, 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.

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 – 108.146 -12.59 0.279 -0.982 1.4 67.666
Hunt & Reffert 2024 108.111 -12.585 0.281 -0.979 1.385 59.3
Cavallo et al. 2024 108.166 -12.612 0.282 – – –
Hunt & Reffert 2023 108.111 -12.585 0.281 -0.979 1.385 59.3

💡 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 – – – – – 279* – –
Cavallo et al. 2024 2.77 1.18 – 115 0.060 – – –
Hunt & Reffert 2023 2.93 1.16 1.27 111 – – – –

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

Visualization

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