IRAS 02130+5509

UTI: UCC Trust Index C_N C_dens C_C3 C_lit C_dup 0.0 0.31 0.38 0.33 1.0
C3	N_50	r_50
BC	23	7.4

Summary

IRAS 02130+5509 is a sparse, loose object of low C3 quality. It is located at a relatively close distance from the Sun, below the mid-plane. It is poorly studied in the literature.

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

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Positions

Reference	RA	DEC	Plx	pmRA	pmDE	Rv
Kharchenko et al. (2012)	34.14	55.397	–	0.72	-0.67	–
Hunt & Reffert (2023)	34.137	55.412	0.567	-0.734	-0.889	–
Cavallo et al. (2024)	34.237	55.261	0.561	–	–	–
Hunt & Reffert (2024)	34.137	55.412	0.567	-0.734	-0.889	–
UCC	34.173	55.353	0.563	-0.737	-0.876	-56.918

Galactocentric position

How are the galactocentric plots generated?

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Estimated members

1 2

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Fundamental parameters

Reference	Values
Kharchenko et al. (2012)	e_bv=0.799, distance=2500, log_age=8.0
Hunt & Reffert (2023)	AV50=0.801, diffAV50=0.963, MOD50=11.184, logAge50=7.516
Cavallo et al. (2024)	AV50=0.75, dMod50=11.09, logAge50=7.4, [Fe/H]50=-0.06
Hunt & Reffert (2024)	MassJ=96.0329, MassTot=154.005

Search coordinates in Bayestar19

Cluster region map