Czernik 16

(OCL 387; FSR 0645; MWSC 282)

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C3
N_50
r_50
AB 136 4.7
Summary

Czernik 16 is a rich, very dense object of high C3 quality. It is located at a moderate distance from the Sun, below the mid-plane. It is well-studied in the literature.

This object shares a moderate percentage of members with a later reported entry.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
Dias et al. (2002) 52.7 52.65 0.29 -3.4
Kharchenko et al. (2012) 52.792 52.632 -2.62 -0.89
Loktin & Popova (2017) 52.785 52.632 -2.38 -1.998
Cantat-Gaudin et al. (2018) 52.754 52.612 0.34 0.795 -2.181
Bica et al. (2019) 52.773 52.603
Soubiran et al. (2018) 52.754 52.612 -30.71
Cantat-Gaudin et al. (2020) 52.754 52.612 0.34 0.795 -2.181
Dias et al. (2021) 52.756 52.609 0.335 0.777 -2.205
Hunt & Reffert (2023) 52.766 52.611 0.377 0.787 -2.221
Cavallo et al. (2024) 52.768 52.585 0.376
Hunt & Reffert (2024) 52.766 52.611 0.377 0.787 -2.221
Almeida et al. (2025) 52.756 52.609
           
UCC 52.755 52.598 0.376 0.785 -2.208 -33.549
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

Explore data in Colab

Fundamental parameters

Reference Values
Dias et al. (2002) E(B-V)=1.29, Dist=2580.0, Age=8.3
Kharchenko et al. (2012) e_bv=1.149, distance=2700, log_age=7.3
Loktin & Popova (2017) E(B-V)=0.78, Dist=1560, logt=8.3
Cantat-Gaudin et al. (2018) dmode=2706.6
Soubiran et al. (2018) dmode=2706.6
Cantat-Gaudin et al. (2020) AVNN=2.61, DistPc=2751.0, AgeNN=8.51
Dias et al. (2021) Av=2.793, Dist=2273, logage=8.526, [Fe/H]=-0.057
Hunt & Reffert (2023) AV50=3.107, diffAV50=1.449, MOD50=11.928, logAge50=7.919
Cavallo et al. (2024) AV50=3.08, dMod50=12.2, logAge50=8.17, [Fe/H]50=0.57
Hunt & Reffert (2024) MassJ=919.730, MassTot=1009.13
Almeida et al. (2025) AV=2.793, Dist=2273, logAge=8.526, MassRk=505.7

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
OC 0270 30.9 52.76 52.62 0.38 0.8 -2.22 0.0