ASCC 70

(MWSC 2010; Alessi 38)

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C3
N_50
r_50
DC 41 5.9
Summary

ASCC 70 is a poorly populated, 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.

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Positions

Reference RA DEC Plx pmRA pmDE Rv
Dias et al. (2002) 183.75 -64.43 -4.99 1.2 -10.44
Kharchenko et al. (2005) 183.75 -64.43 -5.55 -0.32 -7.75
Kharchenko et al. (2007) 183.75 -64.43 0.3 -7.75
Piskunov et al. (2008) 183.748 -64.424
Kharchenko et al. (2013) 183.705 -64.4 -6.0 0.31 -7.8
Kharchenko et al. (2016) 183.696 -64.396
Bica et al. (2019) 183.748 -64.424
Just et al. (2023) 183.696 -64.396
           
UCC 183.722 -64.451 0.201 -7.863 1.097 -13.877
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

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Estimated members

ASCC 70 UCC

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Fundamental parameters

Reference Values
Dias et al. (2002) E(B-V)=0.35, Dist=2700.0, Age=6.92
Kharchenko et al. (2005) E(B-V)=0.35, Dist=2700, logt=6.92
Piskunov et al. (2008) E(B-V)=0.35, Dist=2700, logt=6.92, logMA=4.566
Kharchenko et al. (2013) E(B-V)=0.468, d=2652.0, logt=6.92
Kharchenko et al. (2016) E(B-V)=0.468, d=2652.0, logt=6.92
Just et al. (2023) logt=6.92, logmt=3.495

Search coordinates in Bayestar19

Cluster region map