Kronberger 23

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0.15 UTI
0.33
CN
0.1
Cdens
0.5
CC3
0.25
Clit
0.52
Cdup
Core radius and density 2.7 [pc], 0.5 [pc-2]
  • CN 0.33 Poorly populated
  • Cdens 0.1 Very loose
  • CC3 0.5 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 0.52 Likely unique

Overview

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Kronberger 23 is a poorly populated, very loose object of intermediate C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as an intermediate-age cluster (see Parameters). It is poorly studied in the literature, with no articles listed in the last 9 years.

Note: This is likely a unique object, which shares a moderate percentage of members with at least one previously reported entry. See table with shared members information.

Bica et al. (2019)
Web updates in DAML02, some were later removed (2003 to 2010). The Preliminary Amateur Open Cluster Catalog, Version 08/03/2003.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 346.492 60.252 0.331 -3.716 -2.484 -59.293
Sampedro et al. 2017 346.496 60.254 – -0.92 -0.45 –
Dias et al. 2016 346.496 60.254 – – – –
Tadross 2014 346.496 60.254 – – – –
Dias et al. 2014 346.496 60.254 – -4.02 -1.8 –
Bukowiecki et al. 2011 346.592 60.258 – – – –
Kronberger et al. 2006 346.495 60.254 – – – –

💡 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– 2.4 3.865 – 100 – – – –
Dias et al. 2016 3.06 3.47 – 100 – – – –
Tadross 2014 1.74 4.26 – 100 – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
BDSB 42 48.5 346.59 60.26 0.34 -3.77 -2.74 2.56 0.18
BDSB 39 30.3 346.43 60.26 0.32 -3.77 -2.33 – 0.1

💡 Note: The % column shows the percentage of members that Kronberger 23 shares with each listed object.

Visualization

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