HSC 838

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0.30 UTI
0.43
CN
0.3
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad) 1.5 [N/pc2]
  • CN 0.43 Poorly populated
  • Cdens 0.3 Loose
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 838 is a poorly populated, loose object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a metal-rich, young cluster (see Parameters). It was recently reported in the literature.

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

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 99999– 342.564 58.841 0.246 -3.31 -2.0 -64.166
Hunt & Reffert 2024 342.517 58.827 0.262 -3.326 -2.017 -44.469
Cavallo et al. 2024 342.614 58.845 0.253 – – –
Hunt & Reffert 2023 342.517 58.827 0.262 -3.326 -2.017 -44.469

💡 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] Bfrac BSS
UCC 99999– 3.83 2.495 2.15 56 0.730 550 – –
Hunt & Reffert 2024 – – – – – 550(1) – –
Cavallo et al. 2024 4.02 2.39 – 95 0.730 – – –
Hunt & Reffert 2023 3.64 2.60 2.15 18 – – – –

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3663 62.8 342.58 58.85 0.23 -3.28 -1.96 – 0.01

💡 Note: The % column shows the percentage of members that HSC 838 shares with each listed object.

Visualization

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