Alessi 3

(MWSC 1157; FoF 2434; OCSN 137)

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C3
N_50
r_50
AA 268 65.1
Summary

Alessi 3 is a rich, very dense object of very high C3 quality. It is located at a very close distance from the Sun, below the mid-plane. It is very well-studied in the literature.

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Positions

Reference RA DEC Plx pmRA pmDE Rv
Dias et al. (2002) 109.121 -46.685 -11.49 12.37 20.0
Alessi et al. (2003) 109.1 -46.6 -11.5 12.4
Piskunov et al. (2007) 109.086 -46.61
Piskunov et al. (2008) 109.086 -46.61
Kharchenko et al. (2012) 109.05 -46.617 -11.09 12.72
Loktin & Popova (2017) 109.125 -46.685 -1.203 5.537 20.0
Angelo et al. (2019) 109.138 -46.675
Cantat-Gaudin et al. (2018) 109.275 -46.142 3.566 -9.875 11.958
Bica et al. (2019) 109.086 -46.61
Soubiran et al. (2018) 109.275 -46.142 0.2
Liu & Pang (2019) 108.974 -46.05 3.558 -9.829 11.977
Cantat-Gaudin et al. (2020) 109.275 -46.142 3.566 -9.875 11.958
Dias et al. (2021) 109.7 -46.026 3.559 -9.872 12.014 2.314
Tarricq et al. (2022) 109.341 -46.348 3.619 -9.774 11.954
He et al. (2022) 109.09 -46.308 3.611 -9.82 11.958
Qin et al. (2023) 109.18 -46.3 3.59 -9.72 11.92 0.58
Hunt & Reffert (2023) 109.187 -46.68 3.575 -9.793 11.916 0.317
Cavallo et al. (2024) 109.175 -46.154 3.575
Hunt & Reffert (2024) 109.187 -46.68 3.575 -9.793 11.916 0.317
Alfonso et al. (2024) 109.291 -46.194 3.562 -9.852 11.847
Almeida et al. (2025) 109.7 -46.026
           
UCC 109.169 -46.255 3.573 -9.817 11.954 0.451
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)=0.11, Dist=288.0, Age=8.7, [Fe/H]=-0.275
Alessi et al. (2003) E(B-V)=0.11, d_pc=290.0, logt=8.7
Piskunov et al. (2007) E(B-V)=0.11, Dist=288, logt=8.87, logM=1.496
Piskunov et al. (2008) E(B-V)=0.11, Dist=288, logt=8.87, logM=1.718, logMA=1.57
Kharchenko et al. (2012) e_bv=0.11, distance=311, log_age=8.87, metallicity=-0.275
Loktin & Popova (2017) E(B-V)=0.098, Dist=430, logt=8.859
Angelo et al. (2019) dsun=0.26, Age=0.63, Mphot=18
Cantat-Gaudin et al. (2018) dmode=278.1
Soubiran et al. (2018) dmode=278.1
Liu & Pang (2019) Age=0.437, Z=0.25
Cantat-Gaudin et al. (2020) AVNN=0.14, DistPc=297.0, AgeNN=8.8
Dias et al. (2021) Av=0.178, Dist=278, logage=8.902, [Fe/H]=-0.057
Tarricq et al. (2022) Dist=295, logAgeNN=8.8
He et al. (2022) A0=0.5, logAge=8.6
Qin et al. (2023) E(B-V)=0.02, m-M=7.18, logt=8.95
Hunt & Reffert (2023) AV50=0.108, diffAV50=0.435, MOD50=7.142, logAge50=8.796
Cavallo et al. (2024) AV50=0.32, dMod50=7.28, logAge50=8.63, [Fe/H]50=0.44
Hunt & Reffert (2024) MassJ=58.9422, MassTot=130.630
Alfonso et al. (2024) AV=0.14054, MOD=7.36883, logAge=8.85758, Z=-0.0556
Almeida et al. (2025) AV=0.178, Dist=278, logAge=8.902, MassRk=121.6

Search coordinates in Bayestar19

Cluster region map