FSR 1275

(SAI 77; MWSC 1233)

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C3
N_50
r_50
DB 30 3.4
Summary

FSR 1275 is a poorly populated, very dense object of 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) 112.025 -21.796 -1.79 0.06
Froebrich et al. (2007) 112.021 -21.796
Glushkova et al. (2010) 112.026 -21.796
Kharchenko et al. (2012) 112.013 -21.79 -2.91 2.71
Bica et al. (2019) 112.026 -21.8
Hunt & Reffert (2023) 112.02 -21.771 0.424 -2.125 2.208
Cavallo et al. (2024) 112.047 -21.748 0.423
Hunt & Reffert (2024) 112.02 -21.771 0.424 -2.125 2.208
           
UCC 112.032 -21.785 0.422 -2.142 2.195
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)=0.6, Dist=3750.0, Age=9.4
Glushkova et al. (2010) E(B-V)=0.6, Dist=3750.0, Age=9.4
Kharchenko et al. (2012) e_bv=0.666, distance=4541, log_age=9.4
Hunt & Reffert (2023) AV50=1.117, diffAV50=1.021, MOD50=11.687, logAge50=7.41
Cavallo et al. (2024) AV50=1.6, dMod50=12.05, logAge50=7.46, [Fe/H]50=0.22
Hunt & Reffert (2024) MassJ=379.910, MassTot=210.071

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Cluster region map