Kronberger 18

(MWSC 502; DSH J0518.6+3737)

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0.38 UTI
0.3
CN
0.39
Cdens
0.12
CC3
0.55
Clit
1.0
Cdup
Radius (P>50% members) 4.0 [arcmin]
  • CN 0.3 Poorly populated
  • Cdens 0.39 Loose
  • CC3 0.12 Very low quality
  • Clit 0.55 Moderately studied
  • Cdup 1.0 Unique

Overview

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Kronberger 18 is a poorly populated, loose object of very low C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a very young cluster (see Parameters). It is moderately studied in the literature.

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

Relatively close Moderate extinction Very young

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 79.597 37.61 0.295 0.075 -0.237 11.396
Just et al. 2023 79.663 37.631 – – – –
Bica et al. 2019 79.651 37.619 – – – –
Loktin & Popova 2017 79.65 37.625 – -1.183 -2.076 –
Kharchenko et al. 2016 79.663 37.631 – – – –
Dias et al. 2014 79.65 37.625 – -1.55 -5.74 –
Kharchenko et al. 2013 79.672 37.63 – -4.29 -6.7 –
Kharchenko et al. 2012 79.672 37.63 – -4.29 -6.7 –
Kronberger et al. 2006 79.65 37.622 – – – –
Dias et al. 2002 79.65 37.625 – -1.55 -5.74 –

💡 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
Just et al. 2023 – – – 18 – 127 – –
Loktin & Popova 2017 2.62 1.17 – 513 – – – –
Kharchenko et al. 2016 2.70 2.17 – 18 – – – –
Kharchenko et al. 2013 2.70 2.17 – 18 – – – –
Kharchenko et al. 2012 2.70 2.17 – 18 – – – –
Dias et al. 2002 3.25 4.00 – 100 – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
BDSB 68 33.3 79.56 37.56 0.25 0.18 -0.42 -0.14 0.15
CWNU 4000 16.7 79.53 37.49 0.2 0.2 -0.37 -9.66 0.04

💡 Note: The % column shows the percentage of members that Kronberger 18 shares with each listed object.

Visualization

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