Alessi 33

(ASCC 32; MWSC 1069; FoF 2271)

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C3
N_50
r_50
AA 210 18.7
Summary

Alessi 33 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.

This object shares a large percentage of members with 3 later reported entries.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
Dias et al. (2002) 105.496 -26.503 -1.47 2.32
Kharchenko et al. (2005) 105.49 -26.5 -3.39 1.97
Piskunov et al. (2007) 105.489 -26.503
Piskunov et al. (2008) 105.489 -26.503
Kharchenko et al. (2013) 105.525 -26.56 -2.33 4.25
Kharchenko et al. (2016) 105.52 -26.558
Loktin & Popova (2017) 105.495 -26.503 -0.768 0.813
Cantat-Gaudin et al. (2018) 105.714 -26.512 1.23 -3.307 3.477
Bica et al. (2019) 105.499 -26.499
Soubiran et al. (2018) 105.714 -26.512 35.05
Bossini et al. (2019) 105.714 -26.512
Liu & Pang (2019) 105.742 -26.363 1.219 -3.264 3.461
Cantat-Gaudin et al. (2020) 105.714 -26.512 1.23 -3.307 3.477
Dias et al. (2021) 105.711 -26.576 1.24 -3.317 3.475 34.607
He et al. (2022) 105.703 -26.169 1.233 -3.218 3.456
Just et al. (2023) 105.52 -26.558
Cordoni et al. (2023) 105.711 -26.576 1.24 -3.317 3.475
Hunt & Reffert (2023) 105.71 -26.365 1.249 -3.218 3.488 34.107
Cavallo et al. (2024) 105.761 -26.431 1.246
Celli et al. (2024) 105.714 -26.512
Hunt & Reffert (2024) 105.71 -26.365 1.249 -3.218 3.488 34.107
Alfonso et al. (2024) 105.768 -26.563 1.21 -3.201 3.484
Almeida et al. (2025) 105.711 -26.576
           
UCC 105.744 -26.477 1.252 -3.228 3.502 33.096
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)=0.08, Dist=750.0, Age=8.18
Kharchenko et al. (2005) E(B-V)=0.08, Dist=750, logt=8.18
Piskunov et al. (2007) E(B-V)=0.08, Dist=750, logt=8.18, logM=2.198
Piskunov et al. (2008) E(B-V)=0.08, Dist=750, logt=8.18, logM=2.58, logMA=2.907
Kharchenko et al. (2013) E(B-V)=0.079, d=767.0, logt=8.215
Kharchenko et al. (2016) E(B-V)=0.079, d=767.0, logt=8.215
Loktin & Popova (2017) E(B-V)=0.073, Dist=791, logt=8.189
Cantat-Gaudin et al. (2018) dmode=794.6
Soubiran et al. (2018) dmode=794.6
Bossini et al. (2019) AV=0.218, Dist=9.322, logA=7.404, Fe/H=0.0
Liu & Pang (2019) Age=0.019, Z=-0.75
Cantat-Gaudin et al. (2020) AVNN=0.26, DistPc=805.0, AgeNN=7.4
Dias et al. (2021) Av=0.22, Dist=792, logage=7.432, [Fe/H]=-0.003
He et al. (2022) A0=0.1, logAge=7.25
Just et al. (2023) logt=8.215, logmt=2.342
Cordoni et al. (2023) Av=0.22, Dist=9.494, logAge=7.432, [Fe/H]=-0.003, mass-single=2417.39, fbin-tot=0.36, fbss-MS=0.0
Hunt & Reffert (2023) AV50=0.139, diffAV50=0.734, MOD50=9.449, logAge50=7.196
Cavallo et al. (2024) AV50=0.44, dMod50=9.63, logAge50=6.81, [Fe/H]50=-0.28
Celli et al. (2024) Age=25.1, Mc=559.6
Hunt & Reffert (2024) MassJ=272.054, MassTot=287.631
Alfonso et al. (2024) AV=0.25832, MOD=9.52977, logAge=7.38599, Z=-0.0034
Almeida et al. (2025) AV=0.22, Dist=792, logAge=7.432, MassRk=696.8

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 14294 94.8 105.75 -26.5 1.26 -3.22 3.51 32.7 0.06
OC 0408 6.2 105.12 -26.51 1.22 -3.22 3.55 34.95 0.09
OC 0410 3.3 105.73 -27.38 1.2 -3.1 3.48 35.18 0.13