SAI 48

(MWSC 529; Teutsch 37)

UTI: UCC Trust Index C_N C_dens C_C3 C_lit C_dup 0.0 0.11 0.38 0.44 0.4
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.

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.

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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	–
Kharchenko et al. (2013)	81.055	33.477	–	5.08	-5.66	–
Kharchenko et al. (2016)	81.046	33.477	–	–	–	–
Bica et al. (2019)	81.071	33.506	–	–	–	–
Just et al. (2023)	81.046	33.477	–	–	–	–
UCC	80.864	33.487	0.299	-0.148	-1.257	40.832

Galactocentric position

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)=0.31, Dist=1800.0, Age=9.35
Glushkova et al. (2010)	E(B-V)=0.31, Dist=1800.0, Age=9.35
Kharchenko et al. (2012)	E(B-V)=0.799, d=4001.0, logt=8.95
Kharchenko et al. (2013)	E(B-V)=0.799, d=4001.0, logt=8.95
Kharchenko et al. (2016)	E(B-V)=0.799, d=4001.0, logt=8.95
Just et al. (2023)	logt=8.95, logmt=2.805

Search coordinates in Bayestar19

Cluster region map

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