SAI 17

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C3
N_50
r_50
AB 88 1.6
Summary

SAI 17 is a moderately populated, very dense object of high C3 quality. It is located at a large distance from the Sun, below the mid-plane. It is very well-studied in the literature.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
Dias et al. (2002) 35.2 59.185 0.03 -0.32
Glushkova et al. (2010) 35.201 59.185
Kharchenko et al. (2012) 35.212 59.2 0.03 -0.32
Cantat-Gaudin et al. (2018) 35.218 59.188 0.148 -0.123 -0.682
Bica et al. (2019) 35.211 59.187
Soubiran et al. (2018) 35.218 59.188 -35.13
Cantat-Gaudin et al. (2020) 35.218 59.188 0.148 -0.123 -0.682
Dias et al. (2021) 35.211 59.188 0.121 -0.13 -0.683
Hunt & Reffert (2023) 35.222 59.187 0.188 -0.195 -0.667 -35.755
Cavallo et al. (2024) 35.202 59.182 0.181
Hunt & Reffert (2024) 35.222 59.187 0.188 -0.195 -0.667 -35.755
Almeida et al. (2025) 35.211 59.188
Hu & Soubiran (2025) 35.202 59.182
           
UCC 35.21 59.187 0.182 -0.176 -0.674 -35.446
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

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Fundamental parameters

Reference Values
Dias et al. (2002) E(B-V)=0.98, Dist=3800.0, Age=8.9
Glushkova et al. (2010) E(B-V)=0.98, Dist=3800.0, Age=8.9
Kharchenko et al. (2012) e_bv=1.049, distance=4000, log_age=8.9
Cantat-Gaudin et al. (2018) dmode=5661.1
Soubiran et al. (2018) dmode=5661.1
Cantat-Gaudin et al. (2020) AVNN=2.49, DistPc=6065.0, AgeNN=9.07
Dias et al. (2021) Av=3.148, Dist=5452, logage=8.912, [Fe/H]=-0.365
Hunt & Reffert (2023) AV50=3.158, diffAV50=1.717, MOD50=13.26, logAge50=8.661
Cavallo et al. (2024) AV50=3.23, dMod50=13.35, logAge50=8.85, [Fe/H]50=-0.34
Hunt & Reffert (2024) MassJ=1189.27, MassTot=1189.27
Almeida et al. (2025) AV=3.148, Dist=5452, logAge=8.912, MassRk=722.3
Hu & Soubiran (2025) MA22=-0.32, MA23f=-0.36, MA23g=-0.3, MZ23=-0.45, MK24=-0.35, MF24=-0.3

Search coordinates in Bayestar19

Cluster region map