Kronberger 83

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0.59 UTI
0.7
CN
1.0
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 7.1 [N/pc2]
  • CN 0.7 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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Kronberger 83 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a large distance, above the mid-plane, affected by high extinction. It is catalogued as a massive, near-solar metallicity, intermediate-age cluster (see Parameters). It is poorly studied 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)
Bronze 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– 319.596 55.21 0.146 -2.278 -2.516 –
Hunt & Reffert 2024 319.594 55.208 0.139 -2.376 -2.518 -71.342
Cavallo et al. 2024 319.619 55.194 0.135 – – –
Hunt & Reffert 2023 319.594 55.208 0.139 -2.376 -2.518 -71.342
Kronberger et al. 2006 319.597 55.211 – – – –

💡 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– 5.98 3.2 2.4 194 -0.400 3471 – –
Hunt & Reffert 2024 – – – – – 3471(1) – –
Cavallo et al. 2024 5.57 3.34 – 178 -0.400 – – –
Hunt & Reffert 2023 6.39 3.06 2.40 211 – – – –

(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 3550 86.8 319.59 55.21 0.15 -2.26 -2.52 – 0.08

💡 Note: The % column shows the percentage of members that Kronberger 83 shares with each listed object.

Visualization

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