ASCC 110

(MWSC 3234)

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C3
N_50
r_50
AB 54 6.0
Summary

ASCC 110 is a moderately populated, very dense object of high C3 quality. It is located at a relatively close distance from the Sun, above 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) 300.75 33.57 -1.81 -6.49 -2.87
Piskunov et al. (2008) 300.744 33.572
Kharchenko et al. (2012) 300.735 33.57 0.6 -3.93
Cantat-Gaudin et al. (2018) 300.742 33.528 0.497 0.271 -3.132
Bica et al. (2019) 300.754 33.567
Soubiran et al. (2018) 300.742 33.528 -1.09
Cantat-Gaudin et al. (2020) 300.742 33.528 0.497 0.271 -3.132
Dias et al. (2021) 300.772 33.549 0.495 0.278 -3.134 -1.178
Hunt & Reffert (2023) 300.725 33.527 0.49 0.298 -3.159 -5.627
He et al. (2023) 300.577 33.736 0.726 -0.792 -2.556 -24.91
Cavallo et al. (2024) 300.735 33.502 0.502
Hunt & Reffert (2024) 300.725 33.527 0.49 0.298 -3.159 -5.627
Almeida et al. (2025) 300.772 33.549
           
UCC 300.716 33.522 0.504 0.287 -3.165 -2.15
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
Dias et al. (2002) E(B-V)=0.15, Dist=800.0, Age=8.75
Piskunov et al. (2008) E(B-V)=0.15, Dist=800, logt=8.75, logMA=2.199
Kharchenko et al. (2012) e_bv=0.15, distance=852, log_age=8.55
Cantat-Gaudin et al. (2018) dmode=1902.2
Soubiran et al. (2018) dmode=1902.2
Cantat-Gaudin et al. (2020) AVNN=0.75, DistPc=1971.0, AgeNN=8.9
Dias et al. (2021) Av=1.228, Dist=1583, logage=8.795, [Fe/H]=0.14
Hunt & Reffert (2023) AV50=1.329, diffAV50=1.359, MOD50=11.352, logAge50=8.55
He et al. (2023) A0=0.95, m-M=10.7, logA=7.7
Cavallo et al. (2024) AV50=1.53, dMod50=11.28, logAge50=8.62, [Fe/H]50=0.21
Hunt & Reffert (2024) MassJ=489.120, MassTot=625.534
Almeida et al. (2025) AV=1.228, Dist=1583, logAge=8.795, MassRk=250.7

Search coordinates in Bayestar19

Cluster region map