HSC 863

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0.37 UTI
0.35
CN
1.0
Cdens
0.5
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 1.2 [arcmin]
  • CN 0.35 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 863 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a large distance, well above the mid-plane, affected by high extinction. It is catalogued as a metal-poor, intermediate-age 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.

Very distant High extinction Metal-poor Intermediate age

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 – 340.907 64.195 0.137 -1.962 -1.67 -96.328
Hunt & Reffert 2024 340.908 64.194 0.131 -1.97 -1.683 -92.734
Cavallo et al. 2024 340.959 64.178 0.128 – – –
Hunt & Reffert 2023 340.908 64.194 0.131 -1.97 -1.683 -92.734

💡 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 – – – – – 686* – –
Cavallo et al. 2024 8.39 3.92 – 123 -0.690 – – –
Hunt & Reffert 2023 5.96 3.50 1.89 247 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 2940 100.0 340.9 64.19 0.14 -1.96 -1.67 -96.33 0.11

💡 Note: The % column shows the percentage of members that HSC 863 shares with each listed object.

Visualization

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