HSC 2686

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0.16 UTI
0.0
CN
0.05
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 4.1 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.05 Very loose
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 2686 is a sparse, very loose object of high C3 quality. Its parallax locates it at a large distance, below 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.

Very distant Very high extinction Massive Near-solar metallicity Very young

Cavallo et al. (2024)
Bronze sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 229.212 -58.374 0.161 -5.07 -3.514 –
Hunt & Reffert 2024 229.171 -58.374 0.155 -5.093 -3.526 -56.427
Cavallo et al. 2024 229.197 -58.338 0.155 – – –
Hunt & Reffert 2023 229.171 -58.374 0.155 -5.093 -3.526 -56.427

💡 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 – – – – – 1332* – –
Cavallo et al. 2024 4.79 5.47 – 6 0.480 – – –
Hunt & Reffert 2023 6.12 6.18 2.15 11 – – – –

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

Visualization

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