HSC 2860

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0.09 UTI
0.0
CN
0.07
Cdens
0.38
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 6.9 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.07 Very loose
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 2860 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by very high extinction. It is catalogued as a massive, near-solar metallicity, very 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.

Distant Very high extinction Massive Near-solar metallicity Very young

Cavallo et al. (2024)
Silver sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 257.286 -40.593 0.275 -1.238 -2.712 -149.047
Hunt & Reffert 2024 257.297 -40.61 0.268 -1.253 -2.687 -31.991
Cavallo et al. 2024 257.195 -40.584 0.267 – – –
Hunt & Reffert 2023 257.297 -40.61 0.268 -1.253 -2.687 -31.991

💡 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 – – – – – 4161* – –
Cavallo et al. 2024 3.01 5.39 – 7 0.070 – – –
Hunt & Reffert 2023 3.38 5.72 2.93 14 – – – –

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

Visualization

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