Kronberger 25

(J1822.6-1443; MWSC 2901)

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0.71 UTI
0.49
CN
1.0
Cdens
0.75
CC3
0.65
Clit
1.0
Cdup
Radius (P>50% members) 1.2 [arcmin]
  • CN 0.49 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.65 Moderately studied
  • Cdup 1.0 Unique

Overview

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Kronberger 25 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a metal-rich, very young cluster (see Parameters). It is moderately studied in the literature.

Note: This object shares a small percentage of members with at least one entry reported in the same catalogue. See table with shared members information.

Distant High extinction Metal-rich Very young

Almeida et al. (2025)
Mass determination: invalid due to poor quality CMD. Isochrone match: worst fit.

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 – 275.667 -14.725 0.283 -0.324 -1.901 –
Almeida et al. 2025 275.668 -14.723 – – – –
Hunt & Reffert 2024 275.667 -14.724 0.281 -0.328 -1.904 –
Cavallo et al. 2024 275.67 -14.698 0.281 – – –
Hunt & Reffert 2023 275.667 -14.724 0.281 -0.328 -1.904 –
Dias et al. 2021 275.668 -14.723 0.258 -0.385 -1.83 –
Cantat-Gaudin et al. 2020 275.667 -14.727 0.268 -0.343 -1.827 –
Cantat-Gaudin & Anders 2020 275.667 -14.727 0.268 -0.343 -1.827 –
Bica et al. 2019 275.668 -14.732 – – – –
Cantat-Gaudin et al. 2018 275.667 -14.727 0.268 -0.343 -1.827 –
Kronberger et al. 2006 275.666 -14.728 – – – –
Dias et al. 2002 275.667 -14.728 – – – –

💡 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
Almeida et al. 2025 3.45 3.82 – 6 – 191 – –
Hunt & Reffert 2024 – – – – – 944* – –
Cavallo et al. 2024 2.58 3.85 – 25 1.080 – – –
Hunt & Reffert 2023 3.38 4.26 1.50 6 – – – –
Dias et al. 2021 3.45 3.82 – 6 0.229 – – –
Cantat-Gaudin & Anders 2020 3.37 – – – – – – –
Cantat-Gaudin et al. 2018 3.37 – – – – – – –
Dias et al. 2002 1.22 4.09 – 50 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Kharchenko 2 18.4 275.59 -14.61 0.32 -0.25 -1.94 -240.39 0.45

💡 Note: The % column shows the percentage of members that Kronberger 25 shares with each listed object.

Visualization

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