Antalova 2

(MWSC 2610; OCL 1021.1)

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C3
N_50
r_50
BB 60 6.7
Summary

Antalova 2 is a moderately populated, very dense object of intermediate C3 quality. It is located at a relatively close distance from the Sun, near the mid-plane. It is well-studied in the literature.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
Dias et al. (2002) 262.425 -32.483 -0.15 -2.97
Kharchenko et al. (2013) 262.41 -32.48 -5.87 -0.58
Kharchenko et al. (2016) 262.4 -32.48
Cantat-Gaudin et al. (2018) 262.462 -32.541 0.842 2.037 -1.65
Bica et al. (2019) 262.438 -32.553
Cantat-Gaudin et al. (2020) 262.462 -32.541 0.842 2.037 -1.65
Dias et al. (2021) 262.47 -32.522 0.846 2.118 -1.621
Hunt & Reffert (2023) 262.444 -32.551 0.875 2.025 -1.487 -15.549
Cavallo et al. (2024) 262.494 -32.56 0.871
Celli et al. (2024) 262.462 -32.541
Hunt & Reffert (2024) 262.444 -32.551 0.875 2.025 -1.487 -15.549
Almeida et al. (2025) 262.47 -32.522
           
UCC 262.487 -32.551 0.875 2.019 -1.552 -13.825
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)=3.9, Dist=3500.0, Age=9.1
Kharchenko et al. (2013) E(B-V)=3.727, d=1259.0, logt=6.0
Kharchenko et al. (2016) E(B-V)=3.727, d=1259.0, logt=6.0
Cantat-Gaudin et al. (2018) dmode=1148.4
Cantat-Gaudin et al. (2020) AVNN=1.15, DistPc=1056.0, AgeNN=7.08
Dias et al. (2021) Av=1.167, Dist=1079, logage=6.921, [Fe/H]=0.014
Hunt & Reffert (2023) AV50=1.595, diffAV50=1.93, MOD50=10.234, logAge50=6.923
Cavallo et al. (2024) AV50=2.24, dMod50=11.2, logAge50=7.13, [Fe/H]50=-0.97
Celli et al. (2024) Age=12.0, Mc=143.4
Hunt & Reffert (2024) MassJ=174.897, MassTot=184.877
Almeida et al. (2025) AV=1.167, Dist=1079, logAge=6.921, MassRk=106.7

Search coordinates in Bayestar19

Cluster region map