Collinder 416

(NGC 6882; MWSC 3278; OCL 133; FSR 0168; MWSC 3277)

0.79 UTI

0.55

C_N

0.38

C_dens

1.0

C_C3

1.0

C_lit

1.0

C_dup

N₅₀ (P>50% members) 60

Stellar density (N₅₀/rad) 1.9 [N/pc²]

C3 classification AA

C_N 0.55 Moderately populated
C_dens 0.38 Loose
C_C3 1.0 Very high quality
C_lit 1.0 Very well-studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

MOCA 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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Collinder 416 is a moderately populated, loose object of very high C3 quality. Its parallax locates it at a very close distance, near the mid-plane, affected by low extinction. It is catalogued as a low-mass, near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It is very well-studied in the literature.

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

Very close Low extinction Low mass Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as a moving group.

Data

🔍 Search references for Collinder 416 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	99999–	302.864	26.742	2.092	1.782	-9.277	-19.948
Zhang et al.	2024	302.897	26.751	–	–	–	–
Cavallo et al.	2024	303.435	27.142	2.093	–	–	–
Hunt & Reffert	2023	302.897	26.751	2.089	1.719	-9.215	-22.085
Just et al.	2023	302.943	26.807	–	–	–	–
He et al.	2022	302.815	26.656	2.089	1.749	-9.307	–
Sánchez et al.	2020	302.896	26.534	–	-3.145	-5.599	–
Monteiro & Dias	2019	302.905	26.532	–	-3.199	-5.635	2.456
Bica et al.	2019	302.928	26.547	–	–	–	–
Loktin & Popova	2017	302.94	26.812	–	1.6	-9.8	-15.1
Kharchenko et al.	2016	302.943	26.807	–	–	–	–
Dias et al.	2014	302.896	26.534	–	-4.2	-5.25	-17.67
Kharchenko et al.	2013	302.949	26.81	–	0.37	-9.26	-15.1
Gozha et al.	2012	302.946	26.812	–	–	–	–
Piskunov et al.	2008	302.931	26.807	–	–	–	–
Kharchenko et al.	2007	302.94	26.81	–	0.11	–	-15.07
Kharchenko et al.	2005	302.94	26.81	–	1.26	-10.0	-16.69
Chen et al.	2003	302.978	26.578	–	1.6	-9.8	0.7
Dias et al.	2002	302.946	26.812	–	1.6	-9.8	-17.8

💡 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]	B_frac	BSS
UCC	99999–	0.43	0.19	0.91	145	-0.020	6	–	–
Zhang et al.	2024	–	–	–	–	-0.087⁽¹⁾	–	–	–
Cavallo et al.	2024	0.49	0.48	–	81	0.390	–	–	–
Hunt & Reffert	2023	0.46	0.31	0.91	83	–	–	–	–
Just et al.	2023	–	–	–	158	–	8	–	–
He et al.	2022	–	0.40	–	71	–	–	–	–
Monteiro & Dias	2019	1.87	1.92	–	53	0.037	–	–	–
Loktin & Popova	2017	0.34	0.12	–	47	–	–	–	–
Kharchenko et al.	2016	0.43	0.19	–	158	–	–	–	–
Kharchenko et al.	2013	0.43	0.19	–	158	-0.020	–	–	–
Gozha et al.	2012	–	–	–	–	-0.020	3	–	–
Piskunov et al.	2008	0.34	0.06	–	145	–	–	–	–
Kharchenko et al.	2005	0.34	0.06	–	145	–	–	–	–
Chen et al.	2003	0.60	–	–	1440	-0.020⁽¹⁾	–	–	–
Dias et al.	2002	0.43	0.19	–	158	-0.020	–	–	–

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
OCSN 20	88.3	302.88	26.74	2.1	1.81	-9.29	-20.07	0.02

💡 Note: The % column shows the percentage of members that Collinder 416 shares with each listed object.

Visualization

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