Alessi 37

(ASCC 124; MWSC 3663)

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C3
N_50
r_50
AA 129 16.5
Summary

Alessi 37 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) 342.033 46.252 -0.82 -2.75
Kharchenko et al. (2005) 342.03 46.25 1.34 -2.41
Piskunov et al. (2007) 342.026 46.252
Piskunov et al. (2008) 342.026 46.252
Kharchenko et al. (2012) 341.895 46.31 0.41 -0.78
Kharchenko et al. (2013) 341.895 46.31 0.14 -0.78
Kharchenko et al. (2016) 341.888 46.306
Loktin & Popova (2017) 342.03 46.252 -0.82 -2.75
Cantat-Gaudin et al. (2018) 341.961 46.342 1.384 0.351 -1.569
Bica et al. (2019) 342.025 46.252
Soubiran et al. (2018) 341.961 46.342 -10.48
Bossini et al. (2019) 341.942 46.337
Cantat-Gaudin et al. (2020) 341.961 46.342 1.384 0.351 -1.569
Dias et al. (2021) 342.019 46.328 1.375 0.355 -1.579 -10.602
Tarricq et al. (2022) 341.968 46.33 1.411 0.34 -1.669
He et al. (2022) 341.937 46.308 1.414 0.354 -1.677
Just et al. (2023) 341.888 46.306
Hunt & Reffert (2023) 341.971 46.29 1.384 0.335 -1.643 -13.91
Cavallo et al. (2024) 341.898 46.506 1.381
Hunt & Reffert (2024) 341.971 46.29 1.384 0.335 -1.643 -13.91
Zhang et al. (2024) 341.971 46.29
Alfonso et al. (2024) -18.107 46.39 1.354 0.333 -1.705
Almeida et al. (2025) 342.019 46.328
           
UCC 341.958 46.314 1.413 0.352 -1.659 -15.267
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)=0.15, Dist=600.0, Age=8.48
Kharchenko et al. (2005) E(B-V)=0.15, Dist=600, logt=8.48
Piskunov et al. (2007) E(B-V)=0.15, Dist=600, logt=8.48, logM=1.711
Piskunov et al. (2008) E(B-V)=0.15, Dist=600, logt=8.48, logM=2.286, logMA=1.866
Kharchenko et al. (2012) E(B-V)=0.179, d=700.0, logt=8.191
Kharchenko et al. (2013) E(B-V)=0.179, d=700.0, logt=8.195
Kharchenko et al. (2016) E(B-V)=0.179, d=700.0, logt=8.195
Loktin & Popova (2017) E(B-V)=0.15, Dist=511, logt=8.48
Cantat-Gaudin et al. (2018) dmode=707.9
Soubiran et al. (2018) dmode=707.9
Bossini et al. (2019) AV=0.5255, Dist=9.1905, logA=8.0495, Fe/H=0.0
Cantat-Gaudin et al. (2020) AVNN=0.47, DistPc=695.0, AgeNN=8.14
Dias et al. (2021) Av=0.676, Dist=706, logage=8.366, [Fe/H]=0.063
Tarricq et al. (2022) Dist=683, logAgeNN=8.16
He et al. (2022) A0=0.8, logAge=7.9
Just et al. (2023) logt=8.195, logmt=1.581
Hunt & Reffert (2023) AV50=0.411, diffAV50=1.153, MOD50=9.205, logAge50=8.096
Cavallo et al. (2024) AV50=0.58, dMod50=9.31, logAge50=8.31, [Fe/H]50=0.34
Hunt & Reffert (2024) MassJ=331.235, MassTot=646.263
Zhang et al. (2024) [Fe/H]ANN=-0.0648, [Fe/H]MCMC=-0.0276
Alfonso et al. (2024) AV=0.46680, MOD=9.2117, logAge=8.25943, Z=0.06142
Almeida et al. (2025) AV=0.676, Dist=706, logAge=8.366, MassRk=331.1

Search coordinates in Bayestar19

Cluster region map