HSC 2286

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0.23 UTI
0.0
CN
0.41
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 5.8 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.41 Loose
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 2286 is a sparse, loose object of high C3 quality. Its parallax locates it at a relatively close distance, near 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 – 151.095 -55.129 0.513 -5.466 3.7 6.341
Hunt & Reffert 2024 151.03 -55.096 0.516 -5.474 3.688 1.132
Cavallo et al. 2024 151.078 -55.123 0.514 – – –
Hunt & Reffert 2023 151.03 -55.096 0.516 -5.474 3.688 1.132

💡 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 – – – – – 60* – –
Cavallo et al. 2024 1.99 1.57 – 49 -0.470 – – –
Hunt & Reffert 2023 1.83 1.00 0.61 57 – – – –

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

Visualization

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