FSR 1509

(SAI 110; MWSC 1714)

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C3
N_50
r_50
AB 36 0.9
Summary

FSR 1509 is a poorly populated, very dense object of high C3 quality. It is located at a large 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) 147.004 -55.067 -9.71 2.42
Froebrich et al. (2007) 147.037 -55.073
Glushkova et al. (2010) 147.003 -55.067
Kharchenko et al. (2012) 147.005 -55.067 -9.71 2.42
Cantat-Gaudin et al. (2018) 147.006 -55.073 0.233 -4.049 2.723
Bica et al. (2019) 147.05 -55.073
Soubiran et al. (2018) 147.006 -55.073 19.65
Cantat-Gaudin et al. (2020) 147.006 -55.073 0.233 -4.049 2.723
           
UCC 146.998 -55.07 0.178 -4.003 2.791 16.223
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)=1.17, Dist=2080.0, Age=8.75
Glushkova et al. (2010) E(B-V)=1.17, Dist=2080.0, Age=8.75
Kharchenko et al. (2012) e_bv=1.176, distance=2209, log_age=8.85
Cantat-Gaudin et al. (2018) dmode=3818.3
Soubiran et al. (2018) dmode=3818.3
Cantat-Gaudin et al. (2020) AVNN=3.43, DistPc=4203.0, AgeNN=7.79

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Cluster region map