HSC 2814

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0.36 UTI
0.28
CN
1.0
Cdens
0.5
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 4.9 [arcmin]
  • CN 0.28 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.5 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 2814 is a poorly populated, very dense object of intermediate 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, very young cluster (see Parameters). It was recently reported in the literature.

Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.

Relatively 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 – 252.462 -47.286 0.78 0.945 -3.681 -5.279
Hunt & Reffert 2024 252.455 -47.302 0.774 0.986 -3.677 -3.963
Cavallo et al. 2024 252.413 -47.279 0.776 – – –
Hunt & Reffert 2023 252.455 -47.302 0.774 0.986 -3.677 -3.963

💡 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 – – – – – 143* – –
Cavallo et al. 2024 1.29 2.02 – 13 0.490 – – –
Hunt & Reffert 2023 1.22 2.15 2.02 6 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3126 85.7 252.46 -47.29 0.79 0.94 -3.67 -5.28 0.03

💡 Note: The % column shows the percentage of members that HSC 2814 shares with each listed object.

Visualization

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