HSC 754

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0.06 UTI
0.0
CN
0.19
Cdens
0.12
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 14.6 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.19 Very loose
  • CC3 0.12 Very low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 754 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young 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 Young

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 – 320.813 56.037 0.972 -3.891 -3.58 -7.073
Hunt & Reffert 2024 320.801 56.047 0.984 -3.909 -3.57 -14.14
Cavallo et al. 2024 320.945 55.868 0.981 – – –
Hunt & Reffert 2023 320.801 56.047 0.984 -3.909 -3.57 -14.14

💡 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 – – – – – 59* – –
Cavallo et al. 2024 1.07 1.69 – 12 -0.110 – – –
Hunt & Reffert 2023 0.98 1.74 1.63 101 – – – –

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

Visualization

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