Czernik 17

(OCL 378; MWSC 311)

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C3
N_50
r_50
AB 40 2.7
Summary

Czernik 17 is a poorly populated, loose object of high C3 quality. It is located at a large distance from the Sun, well above the mid-plane. It is moderately studied in the literature.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
Dias et al. (2002) 58.1 61.95 -2.3 1.81
Kharchenko et al. (2012) 58.105 61.96 0.17 -2.19
Loktin & Popova (2017) 58.11 61.951 -0.184 -2.905
Bica et al. (2019) 58.126 61.96
Hunt & Reffert (2023) 58.075 61.972 0.139 0.059 -0.103
He et al. (2023) 58.093 61.975 0.142 0.062 -0.104
Cavallo et al. (2024) 58.099 61.969 0.14
Hunt & Reffert (2024) 58.075 61.972 0.139 0.059 -0.103
           
UCC 58.092 61.975 0.142 0.072 -0.079
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

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Estimated members

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Fundamental parameters

Reference Values
Dias et al. (2002) E(B-V)=0.72, Dist=7000.0, Age=8.05
Kharchenko et al. (2012) e_bv=0.75, distance=2900, log_age=8.98
Loktin & Popova (2017) E(B-V)=0.533, Dist=1802, logt=8.8
Hunt & Reffert (2023) AV50=2.369, diffAV50=0.856, MOD50=13.898, logAge50=8.279
He et al. (2023) A0=1.95, m-M=13.45, logA=8.8
Cavallo et al. (2024) AV50=2.07, dMod50=14.17, logAge50=8.24, [Fe/H]50=0.66
Hunt & Reffert (2024) MassJ=624.759, MassTot=715.657

Search coordinates in Bayestar19

Cluster region map