Dias 1

(Alicante 4; Steine 11; MWSC 67)

N_50

r_50

2.4

Summary

Dias 1 is a moderately populated, very dense object of intermediate C3 quality. It is located at a moderate distance from the Sun, above the mid-plane. It is well-studied in the literature.

This object shares a large percentage of members with 2 later reported entries.

Search object in SciX | Simbad

Positions

Reference	RA	DEC	Plx	pmRA	pmDE	Rv
Dias et al. (2002)	10.646	64.068	–	-2.55	-2.0	–
Kharchenko et al. (2012)	10.653	64.06	–	-0.86	1.33	–
Loktin & Popova (2017)	10.65	64.068	–	-0.868	0.911	–
Cantat-Gaudin et al. (2018)	10.63	64.056	0.372	-2.752	-0.523	–
Bica et al. (2019)	10.616	64.045	–	–	–	–
Cantat-Gaudin et al. (2020)	10.63	64.056	0.372	-2.752	-0.523	–
Dias et al. (2021)	10.643	64.066	0.378	-2.751	-0.508	–
Hunt & Reffert (2023)	10.637	64.054	0.366	-2.761	-0.61	-46.472
Cavallo et al. (2024)	10.623	64.047	0.367	–	–	–
Hunt & Reffert (2024)	10.637	64.054	0.366	-2.761	-0.61	-46.472
Almeida et al. (2025)	10.643	64.066	–	–	–	–

UCC	10.623	64.053	0.366	-2.748	-0.579	-46.489

Galactocentric position

How are the galactocentric plots generated?

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Estimated members

1 2 3

Explore data in Colab

Fundamental parameters

Reference	Values
Dias et al. (2002)	`E(B-V)=1.08, Dist=1690.0, Age=7.1`
Kharchenko et al. (2012)	`e_bv=0.937, distance=2186, log_age=7.9`
Loktin & Popova (2017)	`E(B-V)=0.806, Dist=1560, logt=8.27`
Cantat-Gaudin et al. (2018)	`dmode=2491.1`
Cantat-Gaudin et al. (2020)	`AVNN=2.35, DistPc=2608.0, AgeNN=7.48`
Dias et al. (2021)	`Av=2.982, Dist=2627, logage=6.991, [Fe/H]=-0.194`
Hunt & Reffert (2023)	`AV50=3.388, diffAV50=1.47, MOD50=12.06, logAge50=7.323`
Cavallo et al. (2024)	`AV50=2.99, dMod50=11.35, logAge50=8.16, [Fe/H]50=-0.54`
Hunt & Reffert (2024)	`MassJ=724.911, MassTot=724.911`
Almeida et al. (2025)	`AV=2.982, Dist=2627, logAge=6.991, MassRk=371.8`

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Cmg 672	98.7	10.64	64.05	0.35	-2.74	-0.59	-46.49	0.26
OC 0228	39.7	10.64	64.05	0.36	-2.75	-0.62	-46.49	0.0