Toepler 1

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C3
N_50
r_50
AA 92 1.7
Summary

Toepler 1 is a moderately populated, very dense object of very high C3 quality. It is located at a moderate distance from the Sun, above the mid-plane. It is well-studied in the literature.

This object shares a significant percentage of members with 2 later reported entries.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
Dias et al. (2002) 300.325 33.62 -3.49 -7.96
Kronberger et al. (2006) 300.323 33.615
Kharchenko et al. (2012) 300.322 33.615 -2.77 -0.5
Cantat-Gaudin et al. (2018) 300.318 33.615 0.252 -2.349 -5.081
Soubiran et al. (2018) 300.318 33.615 -3.27
Cantat-Gaudin et al. (2020) 300.318 33.615 0.252 -2.349 -5.081
Dias et al. (2021) 300.319 33.615 0.252 -2.355 -5.079
Hunt & Reffert (2023) 300.323 33.613 0.279 -2.349 -5.07 -4.262
Cavallo et al. (2024) 300.325 33.617 0.278
Hunt & Reffert (2024) 300.323 33.613 0.279 -2.349 -5.07 -4.262
Almeida et al. (2025) 300.319 33.615
           
UCC 300.321 33.613 0.277 -2.345 -5.077 -3.384
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)=0.65, Dist=2793.0, Age=7.85
Kharchenko et al. (2012) e_bv=0.625, distance=2088, log_age=8.655
Cantat-Gaudin et al. (2018) dmode=3558.0
Soubiran et al. (2018) dmode=3558.0
Cantat-Gaudin et al. (2020) AVNN=1.93, DistPc=3454.0, AgeNN=7.81
Dias et al. (2021) Av=2.216, Dist=3111, logage=7.785, [Fe/H]=0.135
Hunt & Reffert (2023) AV50=2.358, diffAV50=1.484, MOD50=12.539, logAge50=8.072
Cavallo et al. (2024) AV50=2.4, dMod50=12.12, logAge50=8.35, [Fe/H]50=-0.16
Hunt & Reffert (2024) MassJ=959.663, MassTot=1002.96
Almeida et al. (2025) AV=2.216, Dist=3111, logAge=7.785, MassRk=258.2

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
OC 0099 64.1 300.32 33.61 0.28 -2.34 -5.07 -3.05 0.01
OC 0098 27.2 300.32 33.62 0.27 -2.33 -5.1 -3.38 0.0