HSC 862

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0.40 UTI
0.25
CN
1.0
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 6.4 [arcmin]
  • CN 0.25 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 862 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It was recently reported in the literature.
Close Moderate extinction Near-solar metallicity Very 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 – 342.75 62.469 1.181 -2.697 -3.518 -3.557
Hunt & Reffert 2024 342.757 62.51 1.179 -2.72 -3.452 -11.21
Cavallo et al. 2024 342.698 62.388 1.185 – – –
Hunt & Reffert 2023 342.757 62.51 1.179 -2.72 -3.452 -11.21

💡 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 – – – – – 73* – –
Cavallo et al. 2024 1.02 3.23 – 9 0.020 – – –
Hunt & Reffert 2023 0.81 2.75 1.62 6 – – – –

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

Visualization

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