NGC 133

UTI: UCC Trust Index C_N C_dens C_C3 C_lit C_dup 0.52 1.0 1.0 0.8 1.0 NGC 133 is a moderately populated, very dense object of very high C3 quality. It is well-studied in the literature. This object shares a large percentage of members with a later reported entry.
C3	N_50	r_50
AA	54	1.6

Search object in SciX | Simbad

Positions

Reference	RA	DEC	Plx	pmRA	pmDE	Rv
Dias et al. (2002)	7.829	63.35	–	-0.7	-0.4	–
Kharchenko et al. (2012)	7.819	63.345	–	-1.92	-1.17	–
Loktin & Popova (2017)	7.83	63.35	–	-3.456	-2.2	–
Dias et al. (2021)	7.832	63.358	0.223	-2.324	-0.41	-86.916
Jaehnig et al. (2021)	7.828	63.372	0.28	-2.55	-0.434	–
Hunt & Reffert (2023)	7.801	63.386	0.222	-2.423	-0.5	-86.441
Cavallo et al. (2024)	7.798	63.387	0.224	–	–	–
Hunt & Reffert (2024)	7.801	63.386	0.222	-2.423	-0.5	-86.441
UCC	7.816	63.386	0.224	-2.398	-0.489	-86.699

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Estimated members

1 2

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Fundamental parameters

Reference	Values
Dias et al. (2002)	E(B-V)=0.6, Dist=630.0, Age=7.0
Kharchenko et al. (2012)	e_bv=0.625, distance=1861, log_age=7.3
Loktin & Popova (2017)	E(B-V)=0.632, Dmod=10.921, logt=7.717
Dias et al. (2021)	Av=2.31, Dist=3308, logage=8.201, [Fe/H]=-0.133
Hunt & Reffert (2023)	AV50=2.291, diffAV50=0.546, MOD50=13.051, logAge50=8.202
Cavallo et al. (2024)	AV50=2.32, dMod50=12.75, logAge50=8.46, [Fe/H]50=0.01
Hunt & Reffert (2024)	MassJ=820.933

Search coordinates in Bayestar19

Cluster region

Objects with shared members

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 185	98.1	7.81	63.39	0.22	-2.42	-0.49	-86.7	0.15