LK 10

(Le Duigou-Knodlseder 10; FSR 0233)

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0.66 UTI
0.8
CN
1.0
Cdens
1.0
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 52.8 [N/pc2]
  • CN 0.8 Rich
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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LK 10 is a rich, very dense object of very high C3 quality. Its parallax locates it at a relatively close* distance, near the mid-plane, affected by very high extinction. It is catalogued as a massive, metal-rich, intermediate-age cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~1.59 kpc) differs significantly from the median photometric distance (~2.52 kpc).

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

Cavallo et al. (2024)
Wood 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– 309.825 40.002 0.627 -2.9 -4.503 13.381
Hunt & Reffert 2024 309.835 39.996 0.613 -2.921 -4.5 12.654
Cavallo et al. 2024 309.831 40.013 0.599 – – –
Hunt & Reffert 2023 309.835 39.996 0.613 -2.921 -4.5 12.654
Bica et al. 2019 309.805 39.98 – – – –

💡 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– 2.525 6.17 2.16 330 0.550 1331 – –
Hunt & Reffert 2024 – – – – – 1331(1) – –
Cavallo et al. 2024 3.61 5.59 – 447 0.550 – – –
Hunt & Reffert 2023 1.44 6.75 2.16 213 – – – –

(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 3942 82.5 309.83 40.01 0.63 -2.91 -4.51 13.38 0.0

💡 Note: The % column shows the percentage of members that LK 10 shares with each listed object.

Visualization

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