ASCC 17

(MWSC 534)

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C3
N_50
r_50
DC 15 5.1
Summary

ASCC 17 is a sparse, very loose object of very low C3 quality. It is located at a moderate distance from the Sun, below the mid-plane. It is moderately studied in the literature.

Warning: contains less than 25 stars with P>0.5 estimated.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
Dias et al. (2002) 81.3 30.17 2.55 -3.74 -16.0
Kharchenko et al. (2005) 81.3 30.17 1.33 -6.39 -16.0
Kharchenko et al. (2007) 81.3 30.17 0.25 -16.0
Piskunov et al. (2008) 81.29 30.167
Kharchenko et al. (2012) 81.33 30.182 2.57 -3.15 -16.0
Kharchenko et al. (2013) 81.33 30.182 2.57 -3.15 -16.0
Kharchenko et al. (2016) 81.321 30.183
Bica et al. (2019) 81.3 30.173
Just et al. (2023) 81.321 30.183
           
UCC 81.328 30.116 0.227 0.099 -0.364 12.568
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

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Estimated members

ASCC 17 UCC

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Fundamental parameters

Reference Values
Dias et al. (2002) E(B-V)=0.32, Dist=2000.0, Age=7.12
Kharchenko et al. (2005) E(B-V)=0.32, Dist=2000, logt=7.12
Piskunov et al. (2008) E(B-V)=0.32, Dist=2000, logt=7.12, logMA=3.393
Kharchenko et al. (2012) E(B-V)=0.371, d=1850.0, logt=7.265
Kharchenko et al. (2013) E(B-V)=0.371, d=1850.0, logt=7.265
Kharchenko et al. (2016) E(B-V)=0.371, d=1850.0, logt=7.265
Just et al. (2023) logt=7.265, logmt=2.514

Search coordinates in Bayestar19

Cluster region map