FSR 1586

(SAI 115; MWSC 1938)

N_50

r_50

215

2.5

Summary

FSR 1586 is a rich, very dense object of very high C3 quality. It is located at a moderate distance from the Sun, below the mid-plane. It is well-studied in the literature.

This object shares a small percentage of members with a later reported entry.

Search object in SciX | Simbad

Positions

Reference	RA	DEC	Plx	pmRA	pmDE	Rv
Dias et al. (2002)	170.688	-62.318	–	-2.83	-4.71	–
Froebrich et al. (2007)	170.704	-62.321	–	–	–	–
Glushkova et al. (2010)	170.687	-62.318	–	–	–	–
Kharchenko et al. (2012)	170.67	-62.32	–	-7.16	5.01	–
Cantat-Gaudin et al. (2018)	170.679	-62.302	0.211	-5.934	1.513	–
Bica et al. (2019)	170.702	-62.322	–	–	–	–
Soubiran et al. (2018)	170.679	-62.302	–	–	–	-8.08
Cantat-Gaudin et al. (2020)	170.679	-62.302	0.211	-5.934	1.513	–
Hunt & Reffert (2023)	170.675	-62.316	0.208	-5.94	1.425	-2.582
Cavallo et al. (2024)	170.682	-62.31	0.205	–	–	–
Hunt & Reffert (2024)	170.675	-62.316	0.208	-5.94	1.425	-2.582

UCC	170.679	-62.315	0.206	-5.941	1.444	-2.005

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)=1.6, Dist=2420.0, Age=8.65`
Glushkova et al. (2010)	`E(B-V)=1.6, Dist=2420.0, Age=8.65`
Kharchenko et al. (2012)	`e_bv=1.603, distance=2863, log_age=8.7`
Cantat-Gaudin et al. (2018)	`dmode=4162.6`
Soubiran et al. (2018)	`dmode=4162.6`
Hunt & Reffert (2023)	`AV50=3.783, diffAV50=2.572, MOD50=12.955, logAge50=7.5`
Cavallo et al. (2024)	`AV50=3.59, dMod50=12.84, logAge50=8.76, [Fe/H]50=0.39`
Hunt & Reffert (2024)	`MassJ=1270.44, MassTot=1368.31`

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
OC 0563	14.9	170.68	-62.32	0.2	-5.92	1.4	-4.02	0.0