Kronberger 53

(DSH J1958.5+3048)

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0.69 UTI
0.82
CN
1.0
Cdens
1.0
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members) 2.3 [arcmin]
  • CN 0.82 Rich
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.31 Poorly studied
  • Cdup 1.0 Unique

Overview

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Kronberger 53 is a rich, very dense object of very 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, young cluster (see Parameters). It is poorly studied in the literature.

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

Distant High extinction Massive Near-solar metallicity Young

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 – 299.639 30.809 0.193 -3.635 -6.02 5.504
Hunt & Reffert 2024 299.645 30.811 0.19 -3.624 -6.018 12.397
Cavallo et al. 2024 299.632 30.805 0.19 – – –
Hunt & Reffert 2023 299.645 30.811 0.19 -3.624 -6.018 12.397
Bica et al. 2019 299.648 30.807 – – – –
Kronberger et al. 2006 299.647 30.811 – – – –

💡 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 – – – – – 4393* – –
Cavallo et al. 2024 3.34 3.47 – 56 -0.380 – – –
Hunt & Reffert 2023 4.78 3.39 2.73 22 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
OC 0091 28.3 299.64 30.81 0.19 -3.63 -6.04 5.79 0.0

💡 Note: The % column shows the percentage of members that Kronberger 53 shares with each listed object.

Visualization

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