HSC 2868

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0.37 UTI
0.37
CN
1.0
Cdens
0.5
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 2.3 [arcmin]
  • CN 0.37 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 2868 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by very high extinction. It is catalogued as a massive, near-solar metallicity, intermediate-age 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.

Relatively close Very high extinction Massive Near-solar metallicity 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 – 258.818 -40.199 0.29 -0.781 -3.006 -36.452
Hunt & Reffert 2024 258.819 -40.197 0.303 -0.79 -3.025 –
Cavallo et al. 2024 258.817 -40.197 0.303 – – –
Hunt & Reffert 2023 258.819 -40.197 0.303 -0.79 -3.025 –

💡 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 – – – – – 1771* – –
Cavallo et al. 2024 2.54 5.15 – 112 -0.480 – – –
Hunt & Reffert 2023 2.92 4.95 2.41 88 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3904 64.9 258.81 -40.2 0.29 -0.79 -3.06 -14.82 0.01

💡 Note: The % column shows the percentage of members that HSC 2868 shares with each listed object.

Visualization

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