SAI 48

(Teutsch 37; MWSC 529)

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C3
N_50
r_50
BC 17 5.8
Summary

SAI 48 is a sparse, very loose object of low C3 quality. It is located at a moderate distance from the Sun, below the mid-plane. It is poorly studied in the literature, with no articles listed in the last 6 years.

Warning: This is possibly a duplicated object, which shares a significant percentage of members with at least one previously reported entry.

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

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
Dias et al. (2002) 81.071 33.501 0.75 -2.45
Glushkova et al. (2010) 81.07 33.501
Kharchenko et al. (2012) 81.055 33.477 5.08 -5.66
Bica et al. (2019) 81.071 33.506
UCC 80.864 33.487 0.299 -0.148 -1.257 40.832
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

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Estimated members

SAI 48 UCC

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Fundamental parameters

Reference Values
Dias et al. (2002) E(B-V)=0.31, Dist=1800.0, Age=9.35
Glushkova et al. (2010) E(B-V)=0.31, Dm=11.3, Age=9.35
Kharchenko et al. (2012) e_bv=0.799, distance=4001, log_age=8.95

Search coordinates in Bayestar19

Cluster region


Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
NGC 1893 60.0 80.73 33.45 0.3 -0.28 -1.41 20.89 0.92