NGC 581

(FoF 2131)

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C3
N_50
r_50
AA 208 3.3
Summary

NGC 581 is a rich, very dense object of very high C3 quality. It is located at a moderate distance from the Sun, below the mid-plane. It is very well-studied in the literature.

This object shares a small percentage of members with 5 later reported entries.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
Dambis (1999) 23.346 60.65
Dias et al. (2002) 23.346 60.65 -1.6 0.66 -44.2
Chen et al. (2003) 23.242 60.662 -1.6 0.66 -37.0
Piskunov et al. (2008) 23.339 60.645
Kharchenko et al. (2012) 23.316 60.652 -1.14 0.37
Loktin & Popova (2017) 23.34 60.65 -0.263 -0.467 -41.4
Cantat-Gaudin et al. (2018) 23.339 60.659 0.373 -1.384 -0.497
Soubiran et al. (2018) 23.339 60.659 -45.33
Bossini et al. (2019) 23.339 60.659
Dias et al. (2019) 23.346 60.65 0.37 -1.382 -0.504 -45.33
Liu & Pang (2019) 23.293 60.638 0.455 -1.367 -0.544
Cantat-Gaudin et al. (2020) 23.339 60.659 0.373 -1.384 -0.497
Dias et al. (2021) 23.331 60.66 0.374 -1.383 -0.493
Rain et al. (2021) 23.339 60.659 0.373 -1.384 -0.497
Jaehnig et al. (2021) 23.331 60.658 0.4 -1.389 -0.504
Hunt & Reffert (2023) 23.36 60.656 0.366 -1.394 -0.598 -38.142
Cavallo et al. (2024) 23.327 60.66 0.366
Celli et al. (2024) 23.339 60.659
Hunt & Reffert (2024) 23.36 60.656 0.366 -1.394 -0.598 -38.142
Almeida et al. (2025) 23.331 60.66
           
UCC 23.341 60.661 0.362 -1.397 -0.581 -38.143
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
Dambis (1999) E_B-V_=0.414, DM0=12.08, log_age_=7.2
Dias et al. (2002) E(B-V)=0.382, Dist=2194.0, Age=7.336
Chen et al. (2003) HDis=2194, Age=0.02
Piskunov et al. (2008) E(B-V)=0.39, Dist=2194, logt=7.44, logMA=2.245
Kharchenko et al. (2012) e_bv=0.331, distance=2199, log_age=7.44
Loktin & Popova (2017) E(B-V)=0.378, Dist=2200, logt=7.337
Cantat-Gaudin et al. (2018) dmode=2487.6
Soubiran et al. (2018) dmode=2487.6
Bossini et al. (2019) AV=1.213, Dist=12.117, logA=7.418, Fe/H=0.0
Dias et al. (2019) E(B-V)=0.34, Dist=2061, logAge=7.336, Z=0.003
Liu & Pang (2019) Age=0.06, Z=0.5
Cantat-Gaudin et al. (2020) AVNN=1.09, DistPc=2502.0, AgeNN=7.44
Dias et al. (2021) Av=1.45, Dist=2292, logage=7.469, [Fe/H]=-0.02
Rain et al. (2021) E(B-V)=0.38, Dist=2487.6, log(Age)=7.33, NBSS=0
Jaehnig et al. (2021) dmode=2.485
Hunt & Reffert (2023) AV50=1.29, diffAV50=0.93, MOD50=11.994, logAge50=7.671
Cavallo et al. (2024) AV50=1.58, dMod50=12.19, logAge50=7.35, [Fe/H]50=-0.1
Celli et al. (2024) Age=27.5, Mc=725.0
Hunt & Reffert (2024) MassJ=1262.03, MassTot=1262.03
Almeida et al. (2025) AV=1.45, Dist=2292, logAge=7.469, MassRk=831.0

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Schoenball 1 16.3 23.42 60.75 0.23 -1.29 -0.65 -37.74 0.17
Gulliver 16 11.1 23.42 60.75 0.21 -1.28 -0.65 -37.02 0.38
Teutsch J0135.2+6041 9.1 23.44 60.67 0.36 -1.44 -0.61 -38.14 0.09
UBC 186 7.7 23.47 60.66 0.34 -1.34 -0.51 0.15
CWWDL 6155 4.8 23.23 60.63 0.34 -1.26 -0.61 0.05