Haffner 16

(MWSC 1355; OCL 655; ESO 493 20; FSR 1309; FoF 382)

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C3
N_50
r_50
AA 164 1.6
Summary

Haffner 16 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 small percentage of members with 3 later reported entries.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
Dambis (1999) 117.583 -25.467
Dias et al. (2002) 117.583 -25.467 -3.4 2.03 65.8
Kharchenko et al. (2003) 117.57 -25.46 -5.51 0.85
Kharchenko et al. (2005) 117.58 -25.46 -5.51 0.62 65.8
Kharchenko et al. (2007) 117.58 -25.47 0.11 65.8
Piskunov et al. (2008) 117.582 -25.459
Kharchenko et al. (2013) 117.588 -25.457 -3.83 4.06 48.7
Kharchenko et al. (2016) 117.582 -25.454
Loktin & Popova (2017) 117.585 -25.467 -3.4 2.03 48.7
Cantat-Gaudin et al. (2018) 117.586 -25.458 0.293 -2.811 2.991
Bica et al. (2019) 117.582 -25.459
Soubiran et al. (2018) 117.586 -25.458 43.64
Liu & Pang (2019) 117.582 -25.48 0.288 -2.568 2.805
Cantat-Gaudin et al. (2020) 117.586 -25.458 0.293 -2.811 2.991
Dias et al. (2021) 117.587 -25.465 0.3 -2.818 2.995
Rain et al. (2021) 117.586 -25.458 0.293 -2.811 2.991
Jaehnig et al. (2021) 117.585 -25.456 0.312 -2.799 3.008
Just et al. (2023) 117.582 -25.454
Hunt & Reffert (2023) 117.585 -25.456 0.294 -2.78 3.026 76.329
Cavallo et al. (2024) 117.589 -25.465 0.293
Hunt & Reffert (2024) 117.585 -25.456 0.294 -2.78 3.026 76.329
Almeida et al. (2025) 117.587 -25.465
           
UCC 117.585 -25.459 0.29 -2.787 3.028 76.449
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_=0.198, DM0=12.6, log_age_=7.45
Dias et al. (2002) E(B-V)=0.175, Dist=3165.0, Age=7.078, [Fe/H]=-0.111
Kharchenko et al. (2003) E(B-V)=0.18, Dist=3125
Kharchenko et al. (2005) E(B-V)=0.18, Dist=3165, logt=7.51
Piskunov et al. (2008) E(B-V)=0.18, Dist=3165, logt=7.51, logMA=3.096
Kharchenko et al. (2013) E(B-V)=0.25, d=2654.0, logt=7.3, [Fe/H]=-0.111
Kharchenko et al. (2016) E(B-V)=0.25, d=2654.0, logt=7.3
Loktin & Popova (2017) E(B-V)=0.175, Dist=3165, logt=7.078
Cantat-Gaudin et al. (2018) dmode=3104.3
Soubiran et al. (2018) dmode=3104.3
Liu & Pang (2019) Age=0.347, Z=0.25
Cantat-Gaudin et al. (2020) AVNN=0.38, DistPc=3244.0, AgeNN=7.92
Dias et al. (2021) Av=0.75, Dist=2862, logage=7.513, [Fe/H]=-0.16
Rain et al. (2021) E(B-V)=0.17, Dist=3104.3, log(Age)=7.07, NBSS=0
Jaehnig et al. (2021) dmode=3.141
Just et al. (2023) logt=7.3, logmt=1.35
Hunt & Reffert (2023) AV50=0.351, diffAV50=1.013, MOD50=12.329, logAge50=7.997
Cavallo et al. (2024) AV50=0.51, dMod50=12.24, logAge50=7.84, [Fe/H]50=-0.16
Hunt & Reffert (2024) MassJ=446.132, MassTot=445.158
Almeida et al. (2025) AV=0.75, Dist=2862, logAge=7.513, MassRk=347.7

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
OC 0417 21.3 117.58 -25.46 0.28 -2.75 3.03 0.0
FSR 1308 11.6 117.57 -25.46 0.31 -2.83 3.05 0.08
CWNU 2123 7.9 117.48 -25.37 0.32 -2.7 2.89 0.08