Czernik 29

(OCL 595; MWSC 1234)

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0.64 UTI
0.47
CN
1.0
Cdens
0.5
CC3
0.62
Clit
1.0
Cdup
Stellar density (N50/rad) 11.1 [N/pc2]
  • CN 0.47 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.5 Intermediate quality
  • Clit 0.62 Moderately studied
  • Cdup 1.0 Unique

Overview

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Czernik 29 is a poorly populated, very dense object of intermediate 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 moderately studied in the literature.

Note: This object shares a moderate percentage of members with at least one entry reported in the same catalogue. See table with shared members information.

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 99999– 112.106 -15.4 0.24 -1.553 1.322 88.409
Hunt & Reffert 2024 112.095 -15.399 0.254 -1.616 1.25 88.404
Cavallo et al. 2024 112.095 -15.398 0.25 – – –
Hunt & Reffert 2023 112.095 -15.399 0.254 -1.616 1.25 88.404
Cantat-Gaudin et al. 2020 112.1 -15.385 0.235 -1.406 1.354 –
Cantat-Gaudin & Anders 2020 112.1 -15.385 0.235 -1.406 1.354 –
Bica et al. 2019 112.085 -15.386 – – – –
Cantat-Gaudin et al. 2018 112.1 -15.385 0.235 -1.406 1.354 –
Loktin & Popova 2017 112.095 -15.405 – -5.013 4.53 –
Dias et al. 2014 112.075 -15.4 – -3.04 2.18 –
van den Bergh 2006 112.075 -15.4 – – – –
Dias et al. 2002 112.075 -15.4 – -3.04 2.18 –

💡 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– 3.54 1.39 0.49 262 -0.440 455 – –
Hunt & Reffert 2024 – – – – – 455(1) – –
Cavallo et al. 2024 3.06 1.72 – 288 -0.440 – – –
Hunt & Reffert 2023 3.57 1.32 0.49 243 – – – –
Cantat-Gaudin et al. 2020 3.48 1.09 – 151 – – – –
Cantat-Gaudin & Anders 2020 3.80 – – – – – – –
Cantat-Gaudin et al. 2018 3.80 – – – – – – –
Loktin & Popova 2017 3.51 0.81 – 617 – – – –
van den Bergh 2006 4.17 1.49 – 200 – – – –
Dias et al. 2002 3.00 1.46 – 282 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Haffner 10 38.3 112.15 -15.36 0.26 -1.18 1.57 87.99 1.0
HSC 1820 4.3 111.98 -15.4 0.17 -1.51 1.47 – 0.1

💡 Note: The % column shows the percentage of members that Czernik 29 shares with each listed object.

Visualization

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