Miller 1

(MWSC 1668)

0.60 UTI

0.52

C_N

1.0

C_dens

0.5

C_C3

0.5

C_lit

1.0

C_dup

C3 classification BB

Number of members (P>50%) 54

Radius (P>50% members) 1.4 [arcmin]

C_N 0.52 Moderately populated
C_dens 1.0 Very dense
C_C3 0.5 Intermediate quality
C_lit 0.5 Moderately studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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Miller 1 is a moderately populated, very dense object of intermediate C3 quality. Its parallax locates it at a large^* distance, below the mid-plane, affected by high extinction. It is catalogued as a very young cluster, but with a large variance across recent sources for the age parameter (see Parameters). It is moderately studied in the literature.

(*): The parallax distance estimate (~7.70 kpc) differs significantly from the median photometric distance (~3.91 kpc).

Note: This object shares a moderate percentage of members with a later reported entry. See table with shared members information.

Distant High extinction Very young

Data

🔍 Search references for Miller 1 in: SciX Simbad

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Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	141.43	-53.238	0.13	-3.828	3.491	43.286
Hunt & Reffert	2024	141.429	-53.242	0.155	-3.824	3.524	65.717
He et al.	2023	141.431	-53.239	0.12	-3.83	3.477	43.29
Hunt & Reffert	2023	141.429	-53.242	0.155	-3.824	3.524	65.717
Just et al.	2023	141.416	-53.222	–	–	–	–
Kharchenko et al.	2016	141.416	-53.222	–	–	–	–
Dias et al.	2014	141.425	-53.233	–	1.22	-1.94	–
Kharchenko et al.	2013	141.42	-53.225	–	-6.32	9.2	–
Dias et al.	2002	141.425	-53.233	–	1.19	-1.89	–

💡 Note: The UCC values are estimated from its identified members.

Reference	Year	Dist [kpc]	Av [mag]	DAv [mag]	Age [Myr]	[Fe/H] [dex]	Mass [Msun]	Bfr	BSS
Hunt & Reffert	2024	–	–	–	–	–	1228*	–	–
He et al.	2023	7.08	3.40	–	16	–	–	–	–
Hunt & Reffert	2023	6.72	2.56	2.08	121	–	–	–	–
Just et al.	2023	–	–	–	4	–	24	–	–
Kharchenko et al.	2016	2.79	7.42	–	4	–	–	–	–
Kharchenko et al.	2013	2.79	7.42	–	4	–	–	–	–
Dias et al.	2002	3.91	1.18	–	1995	–	–	–	–

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 2228	46.3	141.43	-53.24	0.1	-3.83	3.46	65.72	0.0

💡 Note: The % column shows the percentage of members that Miller 1 shares with each listed object.

Visualization

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