FSR 0542

(MWSC 119)

UTI: UCC Trust Index C_N C_dens C_C3 C_lit C_dup 0.78 1.0 0.75 0.79 1.0
C3	N_50	r_50
AB	175	3.9

Summary

FSR 0542 is a rich, very dense object of high C3 quality. It is located at a moderate distance from the Sun, above the mid-plane. It is well-studied in the literature.

Search object in SciX | Simbad

Positions

Reference	RA	DEC	Plx	pmRA	pmDE	Rv
Dias et al. (2002)	21.471	62.995	–	-1.38	-0.08	–
Froebrich et al. (2007)	21.471	62.995	–	–	–	–
Kharchenko et al. (2012)	21.45	62.985	–	1.22	-2.31	–
Kharchenko et al. (2013)	21.45	62.985	–	1.22	-2.31	–
Kharchenko et al. (2016)	21.439	62.981	–	–	–	–
Cantat-Gaudin et al. (2018)	21.485	63.011	0.271	-2.187	-0.203	–
Soubiran et al. (2018)	21.485	63.011	–	–	–	-63.93
Donor et al. (2020)	21.45	62.985	–	-2.09	-0.11	-74.0
Cantat-Gaudin et al. (2020)	21.485	63.011	0.271	-2.187	-0.203	–
Just et al. (2023)	21.439	62.981	–	–	–	–
Hunt & Reffert (2023)	21.459	62.994	0.255	-2.145	-0.329	-72.054
Cavallo et al. (2024)	21.45	62.995	0.252	–	–	–
Hunt & Reffert (2024)	21.459	62.994	0.255	-2.145	-0.329	-72.054
UCC	21.474	63.003	0.255	-2.157	-0.288	-72.772

Galactocentric position

How are the galactocentric plots generated?

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Estimated members

1 2 3

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Fundamental parameters

Reference	Values
Dias et al. (2002)	E(B-V)=0.833, Dist=1934.0, Age=8.35, [Fe/H]=0.07
Kharchenko et al. (2012)	E(B-V)=0.833, d=1934.0, logt=8.35
Kharchenko et al. (2013)	E(B-V)=0.833, d=1934.0, logt=8.35
Kharchenko et al. (2016)	E(B-V)=0.833, d=1934.0, logt=8.35
Cantat-Gaudin et al. (2018)	dmode=3330.7
Soubiran et al. (2018)	dmode=3330.7
Donor et al. (2020)	Fe/H=-0.23
Cantat-Gaudin et al. (2020)	AVNN=3.24, DistPc=3756.0, AgeNN=8.93
Just et al. (2023)	logt=8.35, logmt=2.036
Hunt & Reffert (2023)	AV50=3.371, diffAV50=2.753, MOD50=12.579, logAge50=7.535
Cavallo et al. (2024)	AV50=4.0, dMod50=12.53, logAge50=8.35, [Fe/H]50=-0.08
Hunt & Reffert (2024)	MassJ=1224.68, MassTot=1224.68

Search coordinates in Bayestar19

Cluster region map