FSR 1518

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.0 0.26 0.38 0.25 1.0
C3
N_50
r_50
CB 23 2.2
Summary

FSR 1518 is a sparse, loose object of low C3 quality. It is located at a large distance from the Sun, above the mid-plane. It is poorly studied in the literature, with no articles listed in the last 13 years.

This object shares a significant percentage of members with a later reported entry.

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) 149.871 -54.518 – -4.09 2.38 –
Froebrich et al. (2007) 149.871 -54.518 – – – –
Kharchenko et al. (2012) 149.88 -54.51 – -4.09 2.38 –
           
UCC 149.845 -54.513 0.151 -4.542 2.578 57.334
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

FSR 1518 UCC

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Fundamental parameters

Reference Values
Dias et al. (2002) E(B-V)=0.625, Dist=1819.0, Age=7.6
Kharchenko et al. (2012) e_bv=0.625, distance=1819, log_age=7.6

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3510 68.0 149.85 -54.51 0.11 -4.5 2.58 64.66 0.22