Kronberger 84

(MWSC 3532; DSH J2135.5+5330)

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0.77 UTI
0.55
CN
1.0
Cdens
0.75
CC3
0.77
Clit
1.0
Cdup
Core radius and density 1.3 [pc], 5.3 [pc-2]
  • CN 0.55 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.77 Well-studied
  • Cdup 1.0 Unique

Overview

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Kronberger 84 is a moderately populated, 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, but with a large variance across recent sources for the age, metallicity, and mass parameters (see Parameters). It is well-studied in the literature.

(*): The parallax distance estimate (~4.73 kpc) differs significantly from the median photometric distance (~2.50 kpc).

Almeida et al. (2025)
Mass determination: intermediate fit. Isochrone match: intermediate fit. Silver sample.

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.63 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.63 (50th percentile).

Hu et al. (2021)
Ellipticities (core, all): e_core=0.2015, e_all=0.0965.

Bica et al. (2019)
Web updates in DAML02, some were later removed (2003 to 2010). Asterisms and cluster alikes by B. Alessi reported in DAML02.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 323.884 53.517 0.211 -2.971 -2.985 -76.129
Hu & Soubiran 2025 323.892 53.519 – – – –
Almeida et al. 2025 323.883 53.518 – – – –
Hunt & Reffert 2024 323.888 53.514 0.194 -2.92 -3.032 -61.546
Cavallo et al. 2024 323.892 53.519 0.195 – – –
Hunt & Reffert 2023 323.888 53.514 0.194 -2.92 -3.032 -61.546
Just et al. 2023 323.905 53.485 – – – –
Dias et al. 2021 323.883 53.518 0.232 -3.087 -2.953 –
Cantat-Gaudin et al. 2020 323.884 53.517 0.225 -3.085 -2.908 –
Cantat-Gaudin & Anders 2020 323.884 53.517 0.225 -3.085 -2.908 –
Soubiran et al. 2018 323.884 53.517 – – – -77.43
Bica et al. 2019 323.884 53.51 – – – –
Cantat-Gaudin et al. 2018 323.884 53.517 0.225 -3.085 -2.908 –
Dib et al. 2018 323.91 53.488 – – – –
Loktin & Popova 2017 323.88 53.514 – -1.426 -0.749 –
Sampedro et al. 2017 323.883 53.514 – -4.74 -0.87 –
Joshi et al. 2016 323.91 53.488 – – – –
Kharchenko et al. 2016 323.905 53.485 – – – –
Tadross 2014 323.883 53.514 – – – –
Dias et al. 2014 323.883 53.514 – -3.11 0.1 –
Kharchenko et al. 2013 323.91 53.488 – -4.26 -0.16 –
Kharchenko et al. 2012 323.884 53.515 – -3.86 0.5 –
Bukowiecki et al. 2011 323.883 53.519 – – – –
Kronberger et al. 2006 323.885 53.514 – – – –
Dias et al. 2002 323.883 53.514 – -3.86 0.5 –

💡 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– 2.5 1.92 1.97 600 -0.272 556 – –
Hu & Soubiran 2025 – – – – -0.200(5) – – –
Almeida et al. 2025 3.40 2.43 – 247 – 328 – –
Hunt & Reffert 2024 4.78 2.80 1.97 110 – 891(1) – –
Cavallo et al. 2024 2.36 2.53 – 525 -0.980 – – –
Hunt & Reffert 2023 4.78 2.80 1.97 110 – – – –
Just et al. 2023 – – – 668 – 28 – –
Dias et al. 2021 3.40 2.43 – 247 -0.272 – – –
Cantat-Gaudin et al. 2020 4.04 1.94 – 288 – – – –
Kounkel et al. 2020 4.91 2.67 – 224 – – – –
Cantat-Gaudin & Anders 2020 3.94 – – – – – – –
Soubiran et al. 2018 3.94 – – – – – – –
Cantat-Gaudin et al. 2018 3.94 – – – – – – –
Dib et al. 2018 1.31 – – 668 – – – –
Loktin & Popova 2017 2.50 0.97 – 562 – – – –
Joshi et al. 2016 1.31 1.71 – 668 – – – –
Kharchenko et al. 2016 1.31 1.71 – 668 – – – –
Tadross 2014 1.07 1.92 – 600 – – – –
Kharchenko et al. 2013 1.31 1.71 – 668 – – – –
Bukowiecki et al. 2012 – – – – – 785 – –
Kharchenko et al. 2012 1.20 1.74 – 631 – – – –
Bukowiecki et al. 2011 1.75(1) 0.69 – 1778 – – – –
Dias et al. 2002 1.07 1.92 – 603 – – – –

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Visualization

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