Alessi 12

(LeDrew 2; MWSC 3404; FoF 2391)

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C3
N_50
r_50
AA 303 29.6
Summary

Alessi 12 is a rich, very dense object of very high C3 quality. It is located at a close 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) 310.95 23.792 4.33 -5.35 -26.0
Alessi et al. (2003) 310.827 23.775 4.3 -5.3
Piskunov et al. (2007) 310.873 23.777
Piskunov et al. (2008) 310.873 23.777
Kharchenko et al. (2012) 310.845 23.785 3.33 -5.28
Loktin & Popova (2017) 310.95 23.792 4.33 -5.35 -26.0
Cantat-Gaudin et al. (2018) 310.875 23.871 1.816 4.303 -4.639
Bica et al. (2019) 310.873 23.777
Soubiran et al. (2018) 310.875 23.871 2.43
Bossini et al. (2019) 310.875 23.871
Liu & Pang (2019) 310.945 23.859 1.828 4.358 -4.645
Cantat-Gaudin et al. (2020) 310.875 23.871 1.816 4.303 -4.639
Dias et al. (2021) 310.903 23.897 1.825 4.329 -4.648 -3.374
Tarricq et al. (2022) 310.771 23.978 1.824 4.333 -4.701
He et al. (2022) 310.911 23.797 1.837 4.315 -4.701
Cordoni et al. (2023) 310.903 23.897 1.825 4.329 -4.648
Hunt & Reffert (2023) 310.871 23.538 1.843 4.277 -4.702 1.244
Cavallo et al. (2024) 310.902 23.873 1.834
Hunt & Reffert (2024) 310.871 23.538 1.843 4.277 -4.702 1.244
Alfonso et al. (2024) 310.848 23.833 1.801 4.273 -4.677
Almeida et al. (2025) 310.903 23.897
           
UCC 310.883 23.786 1.838 4.317 -4.702 1.659
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)=0.08, Dist=537.0, Age=8.1
Alessi et al. (2003) E(B-V)=0.08, d_pc=540.0, logt=8.1
Piskunov et al. (2007) E(B-V)=0.08, Dist=537, logt=7.9, logM=2.415
Piskunov et al. (2008) E(B-V)=0.08, Dist=537, logt=7.9, logM=2.736, logMA=2.567
Kharchenko et al. (2012) e_bv=0.079, distance=543, log_age=7.46
Loktin & Popova (2017) E(B-V)=0.175, Dist=1108, logt=8.377
Cantat-Gaudin et al. (2018) dmode=542.0
Soubiran et al. (2018) dmode=542.0
Bossini et al. (2019) AV=0.215, Dist=8.491, logA=8.089, Fe/H=0.0
Liu & Pang (2019) Age=0.083, Z=0.0
Cantat-Gaudin et al. (2020) AVNN=0.1, DistPc=544.0, AgeNN=8.13
Dias et al. (2021) Av=0.248, Dist=539, logage=8.195, [Fe/H]=-0.023
Tarricq et al. (2022) Dist=537, logAgeNN=8.14
He et al. (2022) A0=0.35, logAge=7.9
Cordoni et al. (2023) Av=0.248, Dist=8.658, logAge=8.195, [Fe/H]=-0.023, mass-single=526.082, fbin-tot=0.229, fbss-MS=0.0
Hunt & Reffert (2023) AV50=0.137, diffAV50=0.916, MOD50=8.59, logAge50=8.086
Cavallo et al. (2024) AV50=0.47, dMod50=8.75, logAge50=7.87, [Fe/H]50=0.04
Hunt & Reffert (2024) MassJ=470.992, MassTot=609.347
Alfonso et al. (2024) AV=0.10352, MOD=8.60211, logAge=8.12242, Z=-0.0201
Almeida et al. (2025) AV=0.248, Dist=539, logAge=8.195, MassRk=416.1

Search coordinates in Bayestar19

Cluster region map