Kronberger 36

(SAI 136)

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0.65 UTI
0.76
CN
1.0
Cdens
0.75
CC3
0.38
Clit
1.0
Cdup
Radius (P>50% members) 2.7 [arcmin]
  • CN 0.76 Rich
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.38 Poorly studied
  • Cdup 1.0 Unique

Overview

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Kronberger 36 is a rich, very dense object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is poorly studied in the literature.

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

Relatively close Moderate extinction Near-solar metallicity Intermediate age

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 – 301.139 35.239 0.378 -2.422 -3.998 7.245
Zhang et al. 2024 301.139 35.236 – – – –
Hunt & Reffert 2024 301.139 35.236 0.379 -2.424 -4.014 –
Cavallo et al. 2024 301.147 35.238 0.383 – – –
Hunt & Reffert 2023 301.139 35.236 0.379 -2.424 -4.014 –
Glushkova et al. 2010 301.149 35.218 – – – –
Kronberger et al. 2006 301.13 35.246 – – – –

💡 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
Zhang et al. 2024 – – – – 0.277* – – –
Hunt & Reffert 2024 – – – – – 860* – –
Cavallo et al. 2024 2.26 2.50 – 186 0.220 – – –
Hunt & Reffert 2023 2.40 2.35 2.31 207 – – – –
Glushkova et al. 2010 1.90 2.36 – 251 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 2845 75.4 301.14 35.24 0.38 -2.41 -4.01 – 0.02
UBC 137 43.3 301.14 35.24 0.39 -2.42 -4.0 – 0.0

💡 Note: The % column shows the percentage of members that Kronberger 36 shares with each listed object.

Visualization

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