Kronberger 23

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0.28 UTI
0.33
CN
0.33
Cdens
0.5
CC3
0.13
Clit
1.0
Cdup
Stellar density (N50/rad) 1.6 [N/pc2]
  • CN 0.33 Poorly populated
  • Cdens 0.33 Loose
  • CC3 0.5 Intermediate quality
  • Clit 0.13 Rarely studied
  • Cdup 1.0 Unique

Overview

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Kronberger 23 is a poorly populated, 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 rarely studied in the literature, with no articles listed in the last 9 years.

Note: This object shares a moderate percentage of members with 2 later reported entries. See table with shared members information.

âš ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

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 – –
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 – – – –
Dias et al. 2002 346.496 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 – – – –
Tadross 2014 1.74 4.26 – 100 – – – –
Dias et al. 2002 3.06 3.47 – 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 0.12
BDSB 39 30.3 346.43 60.26 0.32 -3.77 -2.33 – 0.07

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

Visualization

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