NGC 7235

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C3
N_50
r_50
AA 219 3.4
Summary

NGC 7235 is a rich, very dense object of very high C3 quality. It is located at a moderate distance from the Sun, above the mid-plane. It is very well-studied in the literature.

This object shares a moderate percentage of members with 3 later reported entries.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
Dambis (1999) 333.104 57.27
Dias et al. (2002) 333.104 57.27 -4.03 -2.11 -53.71
Chen et al. (2003) 333.084 57.284 -4.03 -2.11 -52.0
Piskunov et al. (2008) 333.105 57.268
Kharchenko et al. (2012) 333.09 57.265 -4.54 -2.35
Loktin & Popova (2017) 333.105 57.27 -0.688 0.028 -53.7
Cantat-Gaudin et al. (2018) 333.083 57.271 0.259 -3.757 -3.026
Soubiran et al. (2018) 333.083 57.271 -57.12
Bossini et al. (2019) 333.083 57.271
Dias et al. (2019) 333.104 57.27 0.262 -3.777 -3.066 -57.12
Cantat-Gaudin et al. (2020) 333.083 57.271 0.259 -3.757 -3.026
Dias et al. (2021) 333.085 57.275 0.259 -3.718 -3.035
Rain et al. (2021) 333.083 57.271 0.152 -2.381 2.935
Jaehnig et al. (2021) 333.067 57.266 0.287 -3.811 -3.038
Hunt & Reffert (2023) 333.086 57.273 0.277 -3.801 -3.095 -61.989
He et al. (2023) 333.162 57.26 0.199 -3.101 -2.77 -73.94
Cavallo et al. (2024) 333.056 57.278 0.277
Celli et al. (2024) 333.083 57.271
Hunt & Reffert (2024) 333.086 57.273 0.277 -3.801 -3.095 -61.989
Almeida et al. (2025) 333.085 57.275
           
UCC 333.07 57.27 0.268 -3.779 -3.079 -63.394
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
Dambis (1999) E_B-V_=0.939, DM0=12.09, log_age_=7.0
Dias et al. (2002) E(B-V)=0.9, Dist=3330.0, Age=6.9
Chen et al. (2003) HDis=2823, Age=0.01
Piskunov et al. (2008) E(B-V)=0.93, Dist=2823, logt=6.76, logMA=2.358
Kharchenko et al. (2012) e_bv=0.931, distance=2700, log_age=7.3
Loktin & Popova (2017) E(B-V)=0.92, Dist=2823, logt=7.11
Cantat-Gaudin et al. (2018) dmode=3467.1
Soubiran et al. (2018) dmode=3467.1
Bossini et al. (2019) AV=2.516, Dist=13.163, logA=7.006, Fe/H=0.0
Dias et al. (2019) E(B-V)=0.82, Dist=3737, logAge=7.309, Z=0.01
Cantat-Gaudin et al. (2020) AVNN=2.37, DistPc=3951.0, AgeNN=6.97
Dias et al. (2021) Av=2.566, Dist=3158, logage=7.1, [Fe/H]=0.018
Rain et al. (2021) E(B-V)=0.81, Dist=5536.9, log(Age)=7.0, NBSS=0
Jaehnig et al. (2021) dmode=3.518
Hunt & Reffert (2023) AV50=2.601, diffAV50=1.202, MOD50=12.673, logAge50=7.166
He et al. (2023) A0=3.35, m-M=13.2, logA=8.2
Cavallo et al. (2024) AV50=2.48, dMod50=12.59, logAge50=7.77, [Fe/H]50=0.63
Celli et al. (2024) Age=9.3, Mc=1551.8
Hunt & Reffert (2024) MassJ=1881.64, MassTot=1881.64
Almeida et al. (2025) AV=2.566, Dist=3158, logAge=7.1, MassRk=1557.2

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
OC 0171 33.3 333.07 57.27 0.28 -3.81 -3.08 -61.99 0.0
OC 0172 16.4 333.08 57.27 0.29 -3.78 -3.08 -61.99 0.0
OC 0173 11.4 333.1 57.28 0.28 -3.82 -3.12 -61.99 0.0