FSR 0425

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C3
N_50
r_50
BB 17 9.0
Summary

FSR 0425 is a sparse, very loose object of intermediate C3 quality. It is located at a moderate distance from the Sun, near the mid-plane. It is poorly studied in the literature, with no articles listed in the last 13 years.

This object shares a very small percentage of members with at least one entry reported in the same catalogue.

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

Warning: the low UTI value and no obvious signs of duplication (C_dup=1.0) indicates that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
Dias et al. (2002) 348.658 61.284 -0.19 -0.93
Froebrich et al. (2007) 348.658 61.284
Kharchenko et al. (2012) 348.699 61.285 -1.89 -1.21
           
UCC 348.557 61.221 0.348 -4.426 -1.856
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

FSR 0425 UCC

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Fundamental parameters

Reference Values
Dias et al. (2002) E(B-V)=1.208, Dist=2644.0, Age=8.7
Kharchenko et al. (2012) e_bv=1.208, distance=2644, log_age=8.7

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 459 8.0 347.95 60.97 0.33 -4.44 -1.79 -68.97 0.4
FSR 0426 4.0 348.93 61.1 0.31 -4.0 -1.99 -57.02 0.1