HSC 2869

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0.27 UTI
0.25
CN
0.46
Cdens
0.62
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad) 2.3 [N/pc2]
  • CN 0.25 Poorly populated
  • Cdens 0.46 Loose
  • CC3 0.62 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 2869 is a poorly populated, loose 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, young cluster, but with a large variance across recent sources for the age parameter (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.

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– 258.408 -39.845 0.771 2.435 -2.593 0.318
Hunt & Reffert 2024 258.405 -39.841 0.723 2.44 -2.527 16.03
Cavallo et al. 2024 258.381 -39.809 0.738 – – –
Hunt & Reffert 2023 258.405 -39.841 0.723 2.44 -2.527 16.03

💡 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– 1.175 2.665 1.91 79 -0.350 433 – –
Hunt & Reffert 2024 – – – – – 433(1) – –
Cavallo et al. 2024 1.05 2.83 – 138 -0.350 – – –
Hunt & Reffert 2023 1.30 2.50 1.91 20 – – – –

(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 3698 100.0 258.35 -39.81 0.77 2.43 -2.63 -7.82 0.17

💡 Note: The % column shows the percentage of members that HSC 2869 shares with each listed object.

Visualization

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