ASCC 128

(MWSC 3720)

Click to load Aladin Lite
C3
N_50
r_50
AA 89 26.8
Summary

ASCC 128 is a moderately populated, moderately dense object of very high C3 quality. It is located at a close distance from the Sun, near 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) 350.146 54.6 -1.79 -0.18
Kharchenko et al. (2005) 350.14 54.6 -1.08 -1.57
Piskunov et al. (2007) 350.135 54.601
Piskunov et al. (2008) 350.135 54.601
Kharchenko et al. (2012) 350.28 54.67 -1.58 -1.68
Kharchenko et al. (2013) 350.28 54.67 -1.58 -1.68
Kharchenko et al. (2016) 350.273 54.666
Cantat-Gaudin et al. (2018) 349.949 54.435 1.509 1.236 0.186
Bica et al. (2019) 350.135 54.601
Soubiran et al. (2018) 349.949 54.435 -14.91
Bossini et al. (2019) 349.949 54.435
Cantat-Gaudin et al. (2020) 349.949 54.435 1.509 1.236 0.186
Dias et al. (2021) 349.937 54.402 1.507 1.213 0.188
Tarricq et al. (2022) 350.123 54.389 1.518 1.236 0.14
He et al. (2022) 350.001 54.571 1.522 1.255 0.081
Just et al. (2023) 350.273 54.666
Hunt & Reffert (2023) 350.161 54.573 1.503 1.185 0.113 -14.485
Cavallo et al. (2024) 349.281 54.169 1.504
Hunt & Reffert (2024) 350.161 54.573 1.503 1.185 0.113 -14.485
Zhang et al. (2024) 350.161 54.573
Alfonso et al. (2024) -10.197 54.406 1.494 1.236 0.151
Almeida et al. (2025) 349.937 54.402
           
UCC 349.968 54.439 1.523 1.236 0.155 -14.835
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)=0.13, Dist=900.0, Age=8.44
Kharchenko et al. (2005) E(B-V)=0.13, Dist=900, logt=8.44
Piskunov et al. (2007) E(B-V)=0.13, Dist=900, logt=8.44, logM=2.215
Piskunov et al. (2008) E(B-V)=0.13, Dist=900, logt=8.44, logM=2.725, logMA=2.769
Kharchenko et al. (2012) E(B-V)=0.2, d=900.0, logt=8.454
Kharchenko et al. (2013) E(B-V)=0.2, d=900.0, logt=8.454
Kharchenko et al. (2016) E(B-V)=0.2, d=900.0, logt=8.454
Cantat-Gaudin et al. (2018) dmode=650.3
Soubiran et al. (2018) dmode=650.3
Bossini et al. (2019) AV=0.453, Dist=9.047, logA=8.486, Fe/H=0.0
Cantat-Gaudin et al. (2020) AVNN=0.41, DistPc=669.0, AgeNN=8.4
Dias et al. (2021) Av=0.613, Dist=650, logage=8.243, [Fe/H]=0.025
Tarricq et al. (2022) Dist=657, logAgeNN=8.42
He et al. (2022) A0=0.75, logAge=7.85
Just et al. (2023) logt=8.454, logmt=1.67
Hunt & Reffert (2023) AV50=0.325, diffAV50=0.565, MOD50=9.019, logAge50=8.044
Cavallo et al. (2024) AV50=0.45, dMod50=9.16, logAge50=8.19, [Fe/H]50=0.48
Hunt & Reffert (2024) MassJ=102.637, MassTot=375.083
Zhang et al. (2024) [Fe/H]ANN=-0.1310, [Fe/H]MCMC=-0.1155
Alfonso et al. (2024) AV=0.41002, MOD=9.12975, logAge=8.48781, Z=0.02522
Almeida et al. (2025) AV=0.613, Dist=650, logAge=8.243, MassRk=140.9

Search coordinates in Bayestar19

Cluster region map